CONSTELLATIONS, ARA the ALTAR Ara Constellation Is Located in the Southern Sky
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Arxiv:2012.09981V1 [Astro-Ph.SR] 17 Dec 2020 2 O
Contrib. Astron. Obs. Skalnat´ePleso XX, 1 { 20, (2020) DOI: to be assigned later Flare stars in nearby Galactic open clusters based on TESS data Olga Maryeva1;2, Kamil Bicz3, Caiyun Xia4, Martina Baratella5, Patrik Cechvalaˇ 6 and Krisztian Vida7 1 Astronomical Institute of the Czech Academy of Sciences 251 65 Ondˇrejov,The Czech Republic(E-mail: [email protected]) 2 Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetsky pr. 13, 119234, Moscow, Russia 3 Astronomical Institute, University of Wroc law, Kopernika 11, 51-622 Wroc law, Poland 4 Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University, Kotl´aˇrsk´a2, 611 37 Brno, Czech Republic 5 Dipartimento di Fisica e Astronomia Galileo Galilei, Vicolo Osservatorio 3, 35122, Padova, Italy, (E-mail: [email protected]) 6 Department of Astronomy, Physics of the Earth and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University in Bratislava, Mlynsk´adolina F-2, 842 48 Bratislava, Slovakia 7 Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, H-1121 Budapest, Konkoly Thege Mikl´os´ut15-17, Hungary Received: September ??, 2020; Accepted: ????????? ??, 2020 Abstract. The study is devoted to search for flare stars among confirmed members of Galactic open clusters using high-cadence photometry from TESS mission. We analyzed 957 high-cadence light curves of members from 136 open clusters. As a result, 56 flare stars were found, among them 8 hot B-A type ob- jects. Of all flares, 63 % were detected in sample of cool stars (Teff < 5000 K), and 29 % { in stars of spectral type G, while 23 % in K-type stars and ap- proximately 34% of all detected flares are in M-type stars. -
Summer Constellations
Night Sky 101: Summer Constellations The Summer Triangle Photo Credit: Smoky Mountain Astronomical Society The Summer Triangle is made up of three bright stars—Altair, in the constellation Aquila (the eagle), Deneb in Cygnus (the swan), and Vega Lyra (the lyre, or harp). Also called “The Northern Cross” or “The Backbone of the Milky Way,” Cygnus is a horizontal cross of five bright stars. In very dark skies, Cygnus helps viewers find the Milky Way. Albireo, the last star in Cygnus’s tail, is actually made up of two stars (a binary star). The separate stars can be seen with a 30 power telescope. The Ring Nebula, part of the constellation Lyra, can also be seen with this magnification. In Japanese mythology, Vega, the celestial princess and goddess, fell in love Altair. Her father did not approve of Altair, since he was a mortal. They were forbidden from seeing each other. The two lovers were placed in the sky, where they were separated by the Celestial River, repre- sented by the Milky Way. According to the legend, once a year, a bridge of magpies form, rep- resented by Cygnus, to reunite the lovers. Photo credit: Unknown Scorpius Also called Scorpio, Scorpius is one of the 12 Zodiac constellations, which are used in reading horoscopes. Scorpius represents those born during October 23 to November 21. Scorpio is easy to spot in the summer sky. It is made up of a long string bright stars, which are visible in most lights, especially Antares, because of its distinctly red color. Antares is about 850 times bigger than our sun and is a red giant. -
Instruction Manual
1 Contents 1. Constellation Watch Cosmo Sign.................................................. 4 2. Constellation Display of Entire Sky at 35° North Latitude ........ 5 3. Features ........................................................................................... 6 4. Setting the Time and Constellation Dial....................................... 8 5. Concerning the Constellation Dial Display ................................ 11 6. Abbreviations of Constellations and their Full Spellings.......... 12 7. Nebulae and Star Clusters on the Constellation Dial in Light Green.... 15 8. Diagram of the Constellation Dial............................................... 16 9. Precautions .................................................................................... 18 10. Specifications................................................................................. 24 3 1. Constellation Watch Cosmo Sign 2. Constellation Display of Entire Sky at 35° The Constellation Watch Cosmo Sign is a precisely designed analog quartz watch that North Latitude displays not only the current time but also the correct positions of the constellations as Right ascension scale Ecliptic Celestial equator they move across the celestial sphere. The Cosmo Sign Constellation Watch gives the Date scale -18° horizontal D azimuth and altitude of the major fixed stars, nebulae and star clusters, displays local i c r e o Constellation dial setting c n t s ( sidereal time, stellar spectral type, pole star hour angle, the hours for astronomical i o N t e n o l l r f -
First Scientific Results with the VLT in Visitor and Service Modes
No. 98 – December 1999 First Scientific Results with the VLT in Visitor and Service Modes Starting with this issue, The Messenger will regularly include scientific results obtained with the VLT. One of the results reported in this issue is a study of NGC 3603, the most massive visible H II region in the Galaxy, with VLT/ISAAC in the near-infrared Js, H, and Ks-bands and HST/WFPC2 at Hα and [N II] wavelengths. These VLT observations are the most sensitive near-infrared observations made to date of a dense starburst region, allowing one to in- vestigate with unprecedented quality its low-mass stellar population. The sensitivity limit to stars detected in all three bands corresponds to 0.1 M0 for a pre-main-sequence star of age 0.7 Myr. The observations clearly show that sub-solar-mass stars down to at least 0.1 M0 do form in massive starbursts (from B. Brandl, W. Brandner, E.K. Grebel and H. Zinnecker, page 46). Js versus Js–Ks colour-magnitude diagrams of NGC 3603. The left-hand panel contains all stars detected in all three wave- bands in the entire field of view (3.4′×3.4′, or 6 pc × 6 pc); the centre panel shows the field stars at r > 75″ (2.25 pc) around the cluster, and the right-hand panel shows the cluster population within r < 33″ (1pc) with the field stars statistically subtracted. The dashed horizontal line (left-hand panel) indicates the detection limit of the previous most sensitive NIR study (Eisenhauer et al. -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Albuquerque Morning Journal, 01-28-1922 Journal Publishing Company
University of New Mexico UNM Digital Repository Albuquerque Morning Journal 1908-1921 New Mexico Historical Newspapers 1-28-1922 Albuquerque Morning Journal, 01-28-1922 Journal Publishing Company Follow this and additional works at: https://digitalrepository.unm.edu/abq_mj_news Recommended Citation Journal Publishing Company. "Albuquerque Morning Journal, 01-28-1922." (1922). https://digitalrepository.unm.edu/ abq_mj_news/460 This Newspaper is brought to you for free and open access by the New Mexico Historical Newspapers at UNM Digital Repository. It has been accepted for inclusion in Albuquerque Morning Journal 1908-1921 by an authorized administrator of UNM Digital Repository. For more information, please contact [email protected]. CITY CITY EDITION ALBUQUEI UE EDITION xjbnal:II Da or Mull. Hoc a l OlITV-S- I OM) YKAll 1922. j by Carrier Month VOI;. CI.XXII. No. U8. Albuquerque, New Mexico, Saturday, January 28, Single oplc,. 5o INCORPORA TION OF LABOR Romance o U. S. Girl That ACGEPTAKGE C00LI00E SAYS THE G. 0. ? UNIONS RECOMMENDED Angered Hohenzollerns Elided HEfJRYFORD'S IS mm away' Pittsburgh. Ta., Jan. 27. TE (Special.) Poverty poverty due MUSCLE SHOALS WORLO'S B Y COMMITTEE OF SENA to the war has killed the romance of pretty and vivacious Nancy Duchess of I.eishman and the Croy. Ad- There comes from rans the news OFFER IS URGED Accomplishments of the ILL that the duchess is suing the duke ministration Are Reviewed REGULATION OF FINAL VOTE 0 5 POWERS If for divorce, and that what was long considered one of the prettiest By Vice President in In- lovu atiiiiis ot the tune has oeen National Agricultural Confer- ii m shattered. -
The History of Star Formation in the Galactic Young Open Cluster NGC 6231
Triggered Star Formation in a Turbulent ISM Proceedings IAU Symposium No. 237, 2006 c 2007 International Astronomical Union B. G. Elmegreen & J. Palouˇs, eds. doi:10.1017/S1743921307002736 The history of star formation in the Galactic young open cluster NGC 6231 Mario E. van den Ancker1 1European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany e-mail: [email protected] Abstract. We study the star formation history of the galactic young open cluster NGC 6231 using new, deep, wide-field BV RI imaging. Contrary to previous suggestions, we do not find a lack of low-mass cluster members; our derived mass function is compatible with a Salpeter IMF. The star formation history of NGC 6231 appears to be bi-modal, with a first wave of star formation activity 3–5 Myr ago, followed by a new generation of stars forming ∼ 1 Myr ago. Keywords. Star Formation, Pre-main sequence Stars, Open clusters and associations The star formation history of the rich open cluster NGC 6231 has been hotly debated in the literature ever since the suggestion by Eggen (1976) that a violent process must have triggered star formation in the region. In the largest photometric study of the region to date, Sung et al. (1998) suggested an abrupt decrease in the number of low-mass stars in NGC 6231 - giving further credibility to a scenario in which star formation in this region may have been triggered. Interestingly, Reed & Cudworth (2003), recently found that the trajectory of the globular cluster NGC 6397 intersected that of the natal cloud of NGC 6231 around five million years ago - close to the estimated age of NGC 6231 – thus providing a plausible candidate for the triggering mechanism. -
The Fall of the Youngest Planetary Nebula, Hen3-1357
IOP Publishing Submitted in this form to ApJ 3 Sept 2020 Astrophysical Journal ApJ (XXXX) XXXXXX https://doi.org/XXXX/XXXX The Fall of the Youngest Planetary Nebula, Hen3-1357 Bruce Balick1*, Martín A. Guerrero2, Gerardo Ramos-Larios3 1 Department of Astronomy, University of Washington, Seattle, WA 98195-1580, USA 2 Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía S/N, 18008 Granada, Spain 3 Instituto de Astronomía y Meteorología, Universidad de Guadalajara, 44130 Guadalajara, Mexico *Corresponding author: [email protected] Received xxxxxx Accepted for publication xxxxxx Published xxxxxx Abstract The Stingray Nebula, aka Hen3-1357, went undetected until 1990 when bright nebular lines and radio emission were unexpectedly discovered. We report changes in shape and rapid and secular decreases in its nebular emission-line fluxes based on well calibrated images obtained by the Hubble Space Telescope in 1996, 2000, and 2016. Hen3-1357 is now a “recombination nebula”. Keywords: planetary nebulae: Planetary nebulae (1249), Post-asymptotic giant branch stars (2121), Ionization (2068) 1. Introduction Planetary nebulae (“PNe”) consist of stellar gas ejected in winds from the surfaces of post Asymptotic Branch Giant (“AGB”) stars. The winds systematically expose deeper and much hotter interior stellar layers until stellar energetic ultraviolet (“UV”) begins to ionize the ejected gas. The PN radiates a rich, luminous, and readily detectable set of emission lines (e.g., 6) as electron recombinations with H+ and He+ and optical forbidden lines of N+, O+, O++, S+, etc. These lines become increasingly visible by about a millennium after the winds begin as the central star shifts towards higher temperatures > 40 kK. -
Educator's Guide: Orion
Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
Ghost Imaging of Space Objects
Ghost Imaging of Space Objects Dmitry V. Strekalov, Baris I. Erkmen, Igor Kulikov, and Nan Yu Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109-8099 USA NIAC Final Report September 2014 Contents I. The proposed research 1 A. Origins and motivation of this research 1 B. Proposed approach in a nutshell 3 C. Proposed approach in the context of modern astronomy 7 D. Perceived benefits and perspectives 12 II. Phase I goals and accomplishments 18 A. Introducing the theoretical model 19 B. A Gaussian absorber 28 C. Unbalanced arms configuration 32 D. Phase I summary 34 III. Phase II goals and accomplishments 37 A. Advanced theoretical analysis 38 B. On observability of a shadow gradient 47 C. Signal-to-noise ratio 49 D. From detection to imaging 59 E. Experimental demonstration 72 F. On observation of phase objects 86 IV. Dissemination and outreach 90 V. Conclusion 92 References 95 1 I. THE PROPOSED RESEARCH The NIAC Ghost Imaging of Space Objects research program has been carried out at the Jet Propulsion Laboratory, Caltech. The program consisted of Phase I (October 2011 to September 2012) and Phase II (October 2012 to September 2014). The research team consisted of Drs. Dmitry Strekalov (PI), Baris Erkmen, Igor Kulikov and Nan Yu. The team members acknowledge stimulating discussions with Drs. Leonidas Moustakas, Andrew Shapiro-Scharlotta, Victor Vilnrotter, Michael Werner and Paul Goldsmith of JPL; Maria Chekhova and Timur Iskhakov of Max Plank Institute for Physics of Light, Erlangen; Paul Nu˜nez of Coll`ege de France & Observatoire de la Cˆote d’Azur; and technical support from Victor White and Pierre Echternach of JPL. -
The Mythology of the Ara Pacis Augustae: Iconography and Symbolism of the Western Side
Acta Ant. Hung. 55, 2015, 17–43 DOI: 10.1556/068.2015.55.1–4.2 DAN-TUDOR IONESCU THE MYTHOLOGY OF THE ARA PACIS AUGUSTAE: ICONOGRAPHY AND SYMBOLISM OF THE WESTERN SIDE Summary: The guiding idea of my article is to see the mythical and political ideology conveyed by the western side of the Ara Pacis Augustae in a (hopefully) new light. The Augustan ideology of power is in the modest opinion of the author intimately intertwined with the myths and legends concerning the Pri- mordia Romae. Augustus strove very hard to be seen by his contemporaries as the Novus Romulus and as the providential leader (fatalis dux, an expression loved by Augustan poetry) under the protection of the traditional Roman gods and especially of Apollo, the Greek god who has been early on adopted (and adapted) by Roman mythology and religion. Key words: Apollo, Ara, Augustus, Pax Augusta, Roma Aeterna, Saeculum Augustum, Victoria The aim of my communication is to describe and interpret the human figures that ap- pear on the external western upper frieze (e.g., on the two sides of the staircase) of the Ara Pacis Augustae, especially from a mythological and ideological (i.e., defined in the terms of Augustan political ideology) point of view. I have deliberately chosen to omit from my presentation the procession or gathering of human figures on both the Northern and on the Southern upper frieze of the outer wall of the Ara Pacis, since their relationship with the iconography of the Western and of the Eastern outer-upper friezes of this famous monument is indirect, although essential, at least in my humble opinion.