Free Astronomy Magazine May-June 2020

Total Page:16

File Type:pdf, Size:1020Kb

Free Astronomy Magazine May-June 2020 cover EN.qxp_l'astrofilo 27/04/2020 16:36 Page 1 THE FREE MULTIMEDIA MAGAZINE THAT KEEPS YOU UPDATED ON WHAT IS HAPPENING IN SPACE Bi-monthly magazine of scientific and technical information ✶ May-June 2020 BBiioofflluuoorreesscceenntt ppllaanneetsts The star S2 moves according to Einstein’s Relativity Do sub-relativistic meteors exist? www.astropublishing.com ✶✶www.facebook.com/astropublishing [email protected] colophon EN_l'astrofilo 27/04/2020 16:36 Page 2 colophon EN_l'astrofilo 27/04/2020 16:36 Page 3 S U M M A R Y BI-MONTHLY MAGAZINE OF SCIENTIFIC AND TECHNICAL INFORMATION The star S2 moves according to Einstein’s Relativity FREELY AVAILABLE THROUGH Observations made with ESO’s Very Large Telescope (VLT) have revealed for the first time that a star or- THE INTERNET biting the supermassive black hole at the centre of the Milky Way moves just as predicted by Einstein’s general theory of relativity. Its orbit is shaped like a rosette and not like an ellipse as predicted by... May-June 2020 4 Biofluorescent planets The closest potentially habitable rocky exoplanets all orbit around red dwarfs. These types of stars are particularly suitable for hosting Earth-sized planets, but they are also characterized by surface phenom- 10 ena very harmful to life as we know it. Some organisms, however, may be able to adapt to intense... ESO telescope observes exoplanet where it rains iron Researchers using ESO’s Very Large Telescope (VLT) have observed an extreme planet where they suspect it rains iron. The ultra-hot giant exoplanet has a day side where temperatures climb above 2400 degrees 22 Celsius, high enough to vaporise metals. Strong winds carry iron vapour to the cooler night side where... How newborn stars prepare for the birth of planets An international team of astronomers used two of the most powerful radio telescopes in the world to create more than three hundred images of planet-forming disks around very young stars in the Orion 24 Clouds. These images reveal new details about the birthplaces of planets and the earliest stages of star... English edition of the magazine lA’ STROFILO The best evidence for elusive mid-size black hole New data from the NASA/ESA Hubble Space Telescope have provided the strongest evidence yet for Editor in chief mid-sized black holes in the Universe. Hubble confirms that this “intermediate-mass” black hole dwells Michele Ferrara 28 inside a dense star cluster. Intermediate-mass black holes (IMBHs) are a long-sought “missing link” in... Scientific advisor Prof. Enrico Maria Corsini ALMA spots metamorphosing aged star Publisher Astro Publishing di Pirlo L. An international team of astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) Via Bonomelli, 106 captured the very moment when an old star first starts to alter its environment. The star has ejected 25049 Iseo - BS - ITALY high-speed bipolar gas jets which are now colliding with the surrounding material; the age of the... email [email protected] 32 Internet Service Provider Aruba S.p.A. Do sub-relativistic meteors exist? Via San Clemente, 53 24036 Ponte San Pietro - BG - ITALY Estimates produced from satellite data and extrapolations from meteor falls indicate that, every day, a few to a few hundred tons of dust and rock enter the Earth’s atmosphere from outer space. Nobody Copyright knows the precise amount, but it is assumed that all of that material formed in our own Solar System... All material in this magazine is, unless 34 otherwise stated, property of Astro Publishing di Pirlo L. or included with permission of its author. Reproduction or retransmission of the materials, in The strange orbits of ‘Tatooine’ planetary disks whole or in part, in any manner, with- Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found striking orbital out the prior written consent of the geometries in protoplanetary disks around binary stars. While disks orbiting the most compact binary copyright holder, is a violation of copy- star systems share very nearly the same plane, disks encircling wide binaries have orbital planes that are... right law. A single copy of the materi- 44 als available through this course may be made, solely for personal, noncom- mercial use. Users may not distribute such copies to others, whether or not The impact of satellite constellations on astronomical observations in electronic form, whether or not for Astronomers have recently raised concerns about the impact of satellite mega-constellations on scientific a charge or other consideration, with- research. To better understand the effect these constellations could have on astronomical observations, out prior written consent of the copy- ESO commissioned a scientific study of their impact, focusing on observations with ESO telescopes in... right holder of the materials. The 46 publisher makes available itself with having rights for possible not charac- terized iconographic sources. ALMA and Rosetta map the journey of phosphorus Advertising - Administration Phosphorus, present in our DNA and cell membranes, is an essential element for life as we know it. But Astro Publishing di Pirlo L. how it arrived on the early Earth is something of a mystery. Astronomers have now traced the journey Via Bonomelli, 106 of phosphorus from star-forming regions to comets using the combined powers of ALMA and the... 25049 Iseo - BS - ITALY 50 email [email protected] chronicles EN_l'Astrofilo 27/04/2020 16:39 Page 4 4 SPACE CHRONICLES The star S2 moves according to Einstein’s Relativity by ESO bservations made with ESO’s wards in the plane of motion. This Very Large Telescope (VLT) famous effect — first seen in the Ohave revealed for the first orbit of the planet Mercury around time that a star orbiting the super- the Sun — was the first evidence in massive black hole at the centre of favour of General Relativity. One the Milky Way moves just as pre- hundred years later we have now dicted by Einstein’s general theory detected the same effect in the mo- of relativity. Its orbit is shaped like tion of a star orbiting the compact a rosette and not like an ellipse as radio source Sagittarius A* at the predicted by Newton’s theory of centre of the Milky Way. This obser- gravity. This long-sought-after re- vational breakthrough strengthens sult was made possible by increas- the evidence that Sagittarius A* ingly precise measurements over must be a supermassive black hole nearly 30 years, which have enabled of 4 million times the mass of the scientists to unlock the mysteries of Sun,” says Reinhard Genzel, Direc- the behemoth lurking at the heart tor at the Max Planck Institute for of our galaxy. “Einstein’s General Relativity pre- his artist’s impression illustrates dicts that bound orbits of one object T the precession of the star’s orbit, with the effect exaggerated for eas- around another are not closed, as in ier visualisation. [ESO/L. Calçada] Newtonian Gravity, but precess for- MAY-JUNE 2020 chronicles EN_l'Astrofilo 27/04/2020 16:39 Page 5 SPACE CHRONICLES 5 MAY-JUNE 2020 chronicles EN_l'Astrofilo 27/04/2020 16:39 Page 6 6 SPACE CHRONICLES MAY-JUNE 2020 chronicles EN_l'Astrofilo 27/04/2020 16:39 Page 7 SPACE CHRONICLES 7 his simulation shows the orbits T of stars very close to the super- massive black hole at the heart of the Milky Way. One of these stars, named S2, orbits every 16 years and is passing very close to the black hole in May 2018. This is a perfect laboratory to test gravitational physics and specifically Einstein’s general theory of relativity. [ESO/L. Calçada/spaceengine.org] Extraterrestrial Physics (MPE) in Garching, Germany and the archi- tect of the 30-year-long pro- gramme that led to this result. Located 26 000 light-years from the Sun, Sagittarius A* and the dense cluster of stars around it provide a unique laboratory for testing physics in an otherwise unexplored and extreme regime of gravity. One of these stars, S2, sweeps in to- wards the supermassive black hole to a closest distance less than 20 bil- lion kilometres (one hundred and twenty times the distance between the Sun and Earth), making it one of the closest stars ever found in orbit around the massive giant. At its closest approach to the black hole, S2 is hurtling through space at almost three percent of the speed of light, completing an orbit once every 16 years. “After following the star in its orbit for over two and a half decades, our exquisite meas- urements robustly detect S2’s Schwarzschild precession in its path around Sagittarius A*,” says Stefan Gillessen of the MPE, who led the analysis of the measurements pub- lished today in the journal Astron- omy & Astrophysics. Most stars and planets have a non- circular orbit and therefore move closer to and further away from the object they are rotating around. S2’s orbit precesses, meaning that the location of its closest point to the supermassive black hole changes with each turn, such that MAY-JUNE 2020 chronicles EN_l'Astrofilo 27/04/2020 16:39 Page 8 his visible light wide-field view T shows the rich star clouds in the constellation of Sagittarius (the Archer) in the direction of the centre of our Milky Way galaxy. The entire image is filled with vast numbers of stars — but far more remain hidden behind clouds of dust and are only revealed in in- frared images. This view was cre- ated from photographs in red and blue light and forming part of the Digitized Sky Survey 2. The field of view is approximately 3.5 degrees x 3.6 degrees.
Recommended publications
  • A Dynamo Mechanism As the Potential Origin of the Long Cycle in Double Periodic Variables Dominik R
    A&A 602, A109 (2017) Astronomy DOI: 10.1051/0004-6361/201628900 & c ESO 2017 Astrophysics A dynamo mechanism as the potential origin of the long cycle in double periodic variables Dominik R. G. Schleicher and Ronald E. Mennickent Departamento de Astronomía, Facultad Ciencias Físicas y Matemáticas, Universidad de Concepción, Av. Esteban Iturra s/n Barrio Universitario, Casilla 160-C, Concepción, Chile e-mail: [email protected] Received 11 May 2016 / Accepted 9 March 2017 ABSTRACT The class of double period variables (DPVs) consists of close interacting binaries, with a characteristic long period that is an order of magnitude longer than the corresponding orbital period, many of them with a characteristic ratio of approximately 35. We consider here the possibility that the accretion flow is modulated as a result of a magnetic dynamo cycle. Due to the short binary separations, we expect the rotation of the donor star to be synchronized with the rotation of the binary due to tidal locking. We here present a model to estimate the dynamo number and the resulting relation between the activity cycle length and the orbital period, as well as an estimate for the modulation of the mass transfer rate. The latter is based on Applegate’s scenario, implying cyclic changes in the radius of the donor star and thus in the mass transfer rate as a result of magnetic activity. Our model is applied to a sample of 17 systems with known physical parameters, 11 of which also have known modulation periods. In spite of the uncertainties of our simplified framework, the results show a reasonable agreement, indicating that a dynamo interpretation is potentially feasible.
    [Show full text]
  • Annual Report 2010
    Research Institute Leiden Observatory (Onderzoekinstituut Sterrewacht Leiden) Annual Report 2010 Sterrewacht Leiden Faculty of Mathematics and Natural Sciences Leiden University Niels Bohrweg 2 Postbus 9513 2333 CA Leiden 2330 RA Leiden The Netherlands http://www.strw.leidenuniv.nl Cover: In the Sackler Laboratory for Astrophysics, the circumstances in the inter- and circumstellar medium are simulated. In 2010, water was successfully made on icy dust grains by H-atom bombardment, understanding was gained how complex molecules form under the extreme conditions that are typical for space, and experiments are now ongoing that investigate under which conditions the building blocks of life form. The picture shows the lab’s newest setup - MATRI2CES - that has been constructed with the aim to 'unlock the chemistry of the heavens'. An electronic version of this annual report is available on the web at http://www.strw.leidenuniv.nl/research/annualreport.php?node=23 Production Annual Report 2010: A. van der Tang, E. Gerstel, F.P. Israel, J. Lub, M. Israel, E. Deul Sterrewacht Leiden Executive (Directie Onderzoeksinstituut) Director K. Kuijken Wetenschappelijk Directeur Director of Education F.P. Israel Onderwijs Directeur Institute Manager E. Gerstel Instituutsmanager Supervisory Council (Raad van advies) Prof. Dr. Ir. J.A.M. Bleeker (Chair) Dr. B. Baud Drs. J.F. van Duyne Prof. Dr. K. Gaemers Prof. Dr. C. Waelkens CONTENTS Contents: Part I Chapter 1 1.1 Foreword 1 1.2 Obituary Adriaan Blaauw 5 1.3 Obituary Jaap Tinbergen 7 Chapter 2 2.1 Heritage 11 2.2 Extrasolar planets 13 2.3 Circumstellar gas and dust 15 2.4 Chemistry and physics of the interstellar medium 20 2.5 Stars 25 2.6 Galaxies of the Local Group 30 2.7 Nearby galaxies: observations and theory 37 2.8.
    [Show full text]
  • Abstracts of Talks 1
    Abstracts of Talks 1 INVITED AND CONTRIBUTED TALKS (in order of presentation) Milky Way and Magellanic Cloud Surveys for Planetary Nebulae Quentin A. Parker, Macquarie University I will review current major progress in PN surveys in our own Galaxy and the Magellanic clouds whilst giving relevant historical context and background. The recent on-line availability of large-scale wide-field surveys of the Galaxy in several optical and near/mid-infrared passbands has provided unprecedented opportunities to refine selection techniques and eliminate contaminants. This has been coupled with surveys offering improved sensitivity and resolution, permitting more extreme ends of the PN luminosity function to be explored while probing hitherto underrepresented evolutionary states. Known PN in our Galaxy and LMC have been significantly increased over the last few years due primarily to the advent of narrow-band imaging in important nebula lines such as H-alpha, [OIII] and [SIII]. These PNe are generally of lower surface brightness, larger angular extent, in more obscured regions and in later stages of evolution than those in most previous surveys. A more representative PN population for in-depth study is now available, particularly in the LMC where the known distance adds considerable utility for derived PN parameters. Future prospects for Galactic and LMC PN research are briefly highlighted. Local Group Surveys for Planetary Nebulae Laura Magrini, INAF, Osservatorio Astrofisico di Arcetri The Local Group (LG) represents the best environment to study in detail the PN population in a large number of morphological types of galaxies. The closeness of the LG galaxies allows us to investigate the faintest side of the PN luminosity function and to detect PNe also in the less luminous galaxies, the dwarf galaxies, where a small number of them is expected.
    [Show full text]
  • Annual Report 2011
    Research Institute Leiden Observatory (Onderzoekinstituut Sterrewacht Leiden) Annual Report 2011 Sterrewacht Leiden Faculty of Mathematics and Natural Sciences Leiden University Niels Bohrweg 2 Postbus 9513 2333 CA Leiden 2300 RA Leiden The Netherlands http://www.strw.leidenuniv.nl Cover: Galaxy clusters grow by mergers with other clusters and galaxy groups. These mergers create shock waves within the intracluster medium (ICM) that can accelerate particles to extreme energies. In the presence of magnetic fields, relativistic electrons form large regions emitting synchrotron radiation, the so- called radio relics. A prime example of these phenomena can be found in the galaxy cluster 1RXS J0603.3+4214 (z = 0.225), recently discovered comparing radio and X-ray large sky surveys. The deep radio image on the front cover taken with the Giant Metrewave Radio Telescope (India) shows that this cluster hosts a spectacularly large bright 1.9 Mpc radio relic (Courtesy: van Weeren and Röttgering, et al.). Initial numerical simulations (Brüggen, van Weeren, Röttgering) indicate that the 1.9 Mpc shock can be explained as originating from a triple cluster merging. Studying such systems yield information on the physics of magnetic fields and particle acceleration as well properties of gas in merging clusters. An electronic version of this annual report is available on the web at http://www.strw.leidenuniv.nl/research/annualreport.php Production Annual Report 2011: A. van der Tang, E. Gerstel, A.S. Abdullah, H.E. Andrews Mancilla, F.P. Israel, M. Kazandjian, E. Deul Sterrewacht Leiden Executive (Directie Onderzoeksinstituut) Director K. Kuijken Wetenschappelijk Directeur Director of Education P. v.d.Werf Onderwijs Directeur Institute Manager E.
    [Show full text]
  • NRAO Newsletter
    NRAONRAO NewsletterNewsletter The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. January 2003 www.nrao.edu/news/newsletters Number 94 ALMA This fall has been a busy period as construction activities a detailed proposal to bring significant enhancements to the accelerate for the ALMA project. The most visible evidence baseline ALMA. These enhancements may include a of progress is the completion of the first prototype antenna compact array of seven- and twelve-meter antennas to at the ALMA Test Facility (ATF) located at the VLA site. improve imaging with short baselines, additional frequency The VertexRSI antenna erection has been completed and the bands, and a second generation correlator. Choices of antenna is undergoing a period of extensive tests to verify enhancements will depend on the level of Japanese funds its performance. A second antenna, supplied by our available. The ALMA Science Advisory Committee European partners, will be erected at the ATF next year. The (ASAC) has provided the ACC with the science cases and a European antenna, produced by a consortium led by the priority ranking of potential ALMA enhancements. In antic- French company Alcatel, is scheduled to be available for ipation of their entry, the Japanese will bring a prototype tests beginning in June 2003. Construction of the founda- antenna to the ATF in 2003 for tests to verify its suitability tion for this antenna is already underway. for use in the compact array. The ALMA Coordinating Committee (ACC) met with NRAO Director Fred Lo has convened a panel of experts the Japanese at ESO headquarters in Germany to begin from inside NRAO to review the technical details of those negotiations for the possible entry of Japan into the ALMA portions of the ALMA project assigned to North America.
    [Show full text]
  • Astronomy Magazine 2020 Index
    Astronomy Magazine 2020 Index SUBJECT A AAVSO (American Association of Variable Star Observers), Spectroscopic Database (AVSpec), 2:15 Abell 21 (Medusa Nebula), 2:56, 59 Abell 85 (galaxy), 4:11 Abell 2384 (galaxy cluster), 9:12 Abell 3574 (galaxy cluster), 6:73 active galactic nuclei (AGNs). See black holes Aerojet Rocketdyne, 9:7 airglow, 6:73 al-Amal spaceprobe, 11:9 Aldebaran (Alpha Tauri) (star), binocular observation of, 1:62 Alnasl (Gamma Sagittarii) (optical double star), 8:68 Alpha Canum Venaticorum (Cor Caroli) (star), 4:66 Alpha Centauri A (star), 7:34–35 Alpha Centauri B (star), 7:34–35 Alpha Centauri (star system), 7:34 Alpha Orionis. See Betelgeuse (Alpha Orionis) Alpha Scorpii (Antares) (star), 7:68, 10:11 Alpha Tauri (Aldebaran) (star), binocular observation of, 1:62 amateur astronomy AAVSO Spectroscopic Database (AVSpec), 2:15 beginner’s guides, 3:66, 12:58 brown dwarfs discovered by citizen scientists, 12:13 discovery and observation of exoplanets, 6:54–57 mindful observation, 11:14 Planetary Society awards, 5:13 satellite tracking, 2:62 women in astronomy clubs, 8:66, 9:64 Amateur Telescope Makers of Boston (ATMoB), 8:66 American Association of Variable Star Observers (AAVSO), Spectroscopic Database (AVSpec), 2:15 Andromeda Galaxy (M31) binocular observations of, 12:60 consumption of dwarf galaxies, 2:11 images of, 3:72, 6:31 satellite galaxies, 11:62 Antares (Alpha Scorpii) (star), 7:68, 10:11 Antennae galaxies (NGC 4038 and NGC 4039), 3:28 Apollo missions commemorative postage stamps, 11:54–55 extravehicular activity
    [Show full text]
  • And Circumstellar Envelopes of Long Period Variable Stars
    THE STRUCTURE OF HYDROXYL MASERS AND CIRCUMSTELLAR ENVELOPES OF LONG PERIOD VARIABLE STARS. Thesis by Mark Jonathan Reid In Partial Fulfillment of the Requirements For the degree of Doctor of Philosophy California Institute of Technology Pasadena, California 1975 (Submitted October 10, 1975) 1 Copyright © by Mark Jonathan Reid 1975 11 ACKNOWLEDGMENTS Throughout the two years it took to prepare this thesis, I have been helped by many people in a variety of ways. I wish to thank those people who have been so generous with their time, knowledge and effort on my behalf. To my wife, Katherine, I give special thanks for all the support and encouragement she has given me. Her influence and effort are evident throughout the text and in many of the drafted figures. I wi sh to thank my advisor, Duane Muhleman, for supporting the observing program when it seemed to be a lost cause, and for the almost daily assistance he has offered me during my four years of graduate work. The successful running of the VLB experiments was due to the efforts of many people. Duane Muhleman, James Moran, Kenneth Johnston, Phillip Schwartz, Jonathan Romney and Richard Schilizzi were very attentive during the actual observations. Jack Welch and the entire Hat Creek staff did an outstanding job keeping their telescope "on the air" almost every minute of the scheduled time. Peter and Holly Schloerb took a late night, impromptu "vacation" to the Owens Valley observatory to replace a broken video tape recorder and Harry Hardebeck lost that night's sleep modifying and adjusting the new recorder.
    [Show full text]
  • A Serendipitous Survey for Variability Amongst the Massive Stellar Population of Westerlund 1
    Astronomy & Astrophysics manuscript no. 13820 c ESO 2018 April 2, 2018 A serendipitous survey for variability amongst the massive stellar population of Westerlund 1⋆ J. S. Clark1, B. W. Ritchie1,2, and I. Negueruela3 1 Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes MK7 6AA, United Kingdom 2 IBM United Kingdom Laboratories, Hursley Park, Winchester, Hampshire S021 2JN, United Kingdom 3 Departamento de F´ısica, Ingenier´ıa de Sistemas y Teor´ıa de la Se˜nal, Universidad de Alicante, Apdo. 99, 03080 Alicante, Spain Accepted ??? Received ??? ABSTRACT Aims. Massive stars are known to demonstrate significant spectroscopic and photometric variability over a wide range of timescales. However the physical mechanisms driving this behaviour remain poorly understood. Westerlund 1 presents an ideal laboratory for studying these processes in a rich, coeval population of post-main sequence stars and we present a pathfinding study aimed at charac- terising their variability. Methods. To do this we utilised the large body of spectroscopic and photometric data that has accumulated for Wd1 during the past decade of intensive studies, supplemented with the sparser historical observations extending back to the early 1960s. Results. Despite the heterogeneous nature of this dataset, we were able to identify both spectroscopic and photometric variability amongst every class of evolved massive star present within Wd 1. Spectroscopic variability attributable to both wind asphericity and photospheric pulsations was present amongst both the hot and cool hypergiants and the former, also with the Wolf Rayets. Given the limitations imposed by the data, we were unable to determine the physical origin of the wind structure inferred for the OB supergiants, noting that it was present in both single pulsating and binary stars.
    [Show full text]
  • Nova Report 2008-2009
    NOVA REPORT 2008-2009 NOVA REPORTNOVA 2008 - 2009 Illustration on the front cover In the background an artist’s impression of the changing phases of exoplanet CoRoT-1b is shown. The panel shows the phase folded lightcurve of this planet as observed with the CoRoT satellite. In sequence, the planet first transits the star, after which the dayside rotates into view, the planet gets eclipsed by the star, and finally the nightside rotates into view and the planet transits the star again. The nightside hemisphere is consistent with being entirely black, just as seen for the interior planets in our own solar system. The dayside flux is most likely thermal emission (from: Snellen, de Mooij & Albrecht, 2009, Nature 459, 543). Illustrations on the back cover Counter clockwise starting at upper left. 1. The Sloan Great Wall. Top and face-on view of the SDSS DR7 volume within R<300 h-1Mpc. The Sloan Great Wall is the region roughly located in between the grey lines at Y=155-230 h-1Mpc. The location of well known supercluster are indicated, along with prominent underdense regions like the Bahcall-Soneira Rift and the Boötes and Virgo Supervoid. The outline of supervoids that lie in front are shown as dashed circles (from: Platen & van de Weygaert MNRAS, submitted). 2. Spectral scan of the Orion molecular cloud around 1 THz obtained with the Herschel-HIFI instrument built under leadership of SRON, showing strong lines of water and other simple and complex molecules (credit: ESA, HEXOS and the HIFI consortium). Dutch astronomers are using similarly high quality HIFI spectra to investigate the physical and chemical structure of star-forming regions in our own and nearby galaxies.
    [Show full text]
  • The Magnetic Field of the Evolved Star W43A
    A&A 509, A26 (2010) Astronomy DOI: 10.1051/0004-6361/200913194 & c ESO 2010 Astrophysics The magnetic field of the evolved star W43A N. Amiri1,3,W.Vlemmings2, and H. J. van Langevelde3,1 1 Sterrewacht Leiden, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands e-mail: [email protected] 2 Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, 53121 Bonn, Germany 3 Joint Institute for VLBI in Europe (JIVE), Postbus 2, 7990 AA Dwingeloo, The Netherlands Received 27 August 2009 / Accepted 13 October 2009 ABSTRACT Context. The majority of the observed planetary nebulae exhibit elliptical or bipolar structures. Recent observations have shown that asymmetries already start during the last stages of the AGB phase. Theoretical modeling has indicated that magnetically collimated jets may be responsible for the formation of the non-spherical planetary nebulae. Direct measurement of the magnetic field of evolved stars is possible using polarization observations of different maser species occurring in the circumstellar envelopes around these stars. Aims. The aim of this project is to measure the Zeeman splitting caused by the magnetic field in the OH and H2O maser regions occurring in the circumstellar envelope and bipolar outflow of the evolved star W43A. We compare the magnetic field obtained in the OH maser region with the one measured in the H2O maser jet. Methods. We used the UK Multi-Element Radio Linked Interferometer Network (MERLIN) to observe the polarization of the OH masers in the circumstellar envelope of W43A. Likewise, we used the Green Bank Telescope (GBT) observations to measure the magnetic field strength obtained previously in the H2O maser jet.
    [Show full text]
  • A Serendipitous Survey for Variability Amongst the Massive Stellar Population of Westerlund 1,
    A&A 514, A87 (2010) Astronomy DOI: 10.1051/0004-6361/200913820 & c ESO 2010 Astrophysics A serendipitous survey for variability amongst the massive stellar population of Westerlund 1, J. S. Clark1,B.W.Ritchie1,2, and I. Negueruela3 1 Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK e-mail: [email protected] 2 IBM United Kingdom Laboratories, Hursley Park, Winchester, Hampshire S021 2JN, UK 3 Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Apdo. 99, 03080 Alicante, Spain Received 7 December 2009 / Accepted 17 February 2010 ABSTRACT Aims. Massive stars are known to demonstrate significant spectroscopic and photometric variability over a wide range of timescales. However the physical mechanisms driving this behaviour remain poorly understood. Westerlund 1 presents an ideal laboratory for studying these processes in a rich, coeval population of post-main sequence stars and we present a pathfinding study aimed at charac- terising their variability. Methods. To do this we utilised the large body of spectroscopic and photometric data that has accumulated for Wd1 during the past decade of intensive studies, supplemented with the sparser historical observations extending back to the early 1960s. Results. Despite the heterogeneous nature of this dataset, we were able to identify both spectroscopic and photometric variability amongst every class of evolved massive star present within Wd 1. Spectroscopic variability attributable to both wind asphericity and photospheric pulsations was present amongst both the hot and cool hypergiants and the former, also with the Wolf Rayets. Given the limitations imposed by the data, we were unable to determine the physical origin of the wind structure inferred for the OB supergiants, noting that it was present in both single pulsating and binary stars.
    [Show full text]
  • THE NATURE of OH/IR STARS Jaap Herman
    INIS-mf—• 9020 THE NATURE OF OH/IR STARS Properties and characteristics of an evolved stellar population Jaap Herman THE NATURE OF OH/IR STARS properties and characteristics of an evolved stellar population THE NATURE OF OH/IR STARS properties and characteristics of an evolved stellar population proefschrift ter verkrijging van de graad van Doctor in de Wiskunde en Natuurwetenschappen aan de Rijksuniversiteit te Leiden, op gezag van de Rector Magnificus Dr. A.A.H. Kassenaar, hoogleraar in de faculteit der Geneeskunde, volgens besluit van het college van dekanen te verdedigen op donderdag 8 september 1983 te klokke 14.15 uur door Jacobus Herman geboren te Haarlem in 1954 Sterrewacht Leiden 1983 Beugelsdijk Leiden B.V. De beoordelingscommissie bestond uit de volgende leden: Professor dr. H.J. Habing, promotor Dr. J. Lub, referent Dr. L.L.E. Braes, referent Professor dr. W.B. Burton Professor dr. H.C. van de Hulst Professor dr. T. de Jong Professor dr. J.H. van der Waals, q.q. This research was supported by a grant from ASTRON, the Netherlands Foundation for Astronomical Research. ASTRON receives its funds from ZWO, the Netherlands Organization for the Advancement of Pure Research. aan mijn ouders The nature of OH/IR stars Properties and characteristics of an evolved stellar population Contents Contents 7 Summary 11 Chapter I General Introduction I.I History 15 1.2 Present state of knowledge 19 1.3 Means 21 Chapter II Dwingeloo Monitor II.I Introduction 27 II.2 Observations 27 . II.3 Calibration 27 11,4 Reduction 28 II.5 Confusion 30 II.6 Data analysis a.
    [Show full text]