Gemini (Constellation) - Wikipedia, the Free Encyclopedia
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Nitrogen Abundances in Planet-Harbouring Stars
A&A 418, 703–715 (2004) Astronomy DOI: 10.1051/0004-6361:20035717 & c ESO 2004 Astrophysics Nitrogen abundances in planet-harbouring stars A. Ecuvillon1, G. Israelian1,N.C.Santos2,3, M. Mayor3,R.J.Garc´ıa L´opez1,4, and S. Randich5 1 Instituto de Astrof´ısica de Canarias, 38200 La Laguna, Tenerife, Spain 2 Centro de Astronomia e Astrofisica de Universidade de Lisboa, Observatorio Astronomico de Lisboa, Tapada de Ajuda, 1349-018 Lisboa, Portugal 3 Observatoire de Gen`eve, 51 ch. des Maillettes, 1290 Sauverny, Switzerland 4 Departamento de Astrof´ısica, Universidad de La Laguna, Av. Astrof´ısico Francisco S´anchez s/n, 38206 La Laguna, Tenerife, Spain 5 INAF/Osservatorio Astrofisico di Arcetri, Largo Fermi 5, 50125 Firenze, Italy Received 20 November 2003 / Accepted 4 February 2004 Abstract. We present a detailed spectroscopic analysis of nitrogen abundances in 91 solar-type stars, 66 with and 25 without known planetary mass companions. All comparison sample stars and 28 planet hosts were analysed by spectral synthesis of the near-UV NH band at 3360 Å observed at high resolution with the VLT/UVES, while the near-IR N 7468 Å was measured in 31 objects. These two abundance indicators are in good agreement. We found that nitrogen abundance scales with that of iron in the metallicity range −0.6 < [Fe/H] < +0.4 with the slope 1.08 ± 0.05. Our results show that the bulk of nitrogen production at high metallicities was coupled with iron. We found that the nitrogen abundance distribution in stars with exoplanets is the high [Fe/H] extension of the curve traced by the comparison sample of stars with no known planets. -
Three-Year Follow up of the Phase 3 Pollux Study of Daratumumab Plus
This is a repository copy of Three-Year Follow up of the Phase 3 Pollux Study of Daratumumab Plus Lenalidomide and Dexamethasone (D-Rd) Versus Lenalidomide and Dexamethasone (Rd) Alone in Relapsed or Refractory Multiple Myeloma (RRMM). White Rose Research Online URL for this paper: http://eprints.whiterose.ac.uk/157106/ Version: Accepted Version Proceedings Paper: Bahlis, N, Dimopoulos, MA, White, DJ et al. (14 more authors) (2018) Three-Year Follow up of the Phase 3 Pollux Study of Daratumumab Plus Lenalidomide and Dexamethasone (D-Rd) Versus Lenalidomide and Dexamethasone (Rd) Alone in Relapsed or Refractory Multiple Myeloma (RRMM). In: Blood. ASH 2018 – 60th American Society of Hematology Annual Meeting and Exposition, 01-04 Dec 2018, San Diego, CA. American Society of Hematology . https://doi.org/10.1182/blood-2018-99-112697 © 2018 by The American Society of Hematology. This is an author produced version of a conference abstract published in Blood. Uploaded in accordance with the publisher's self-archiving policy. Reuse Items deposited in White Rose Research Online are protected by copyright, with all rights reserved unless indicated otherwise. They may be downloaded and/or printed for private study, or other acts as permitted by national copyright laws. The publisher or other rights holders may allow further reproduction and re-use of the full text version. This is indicated by the licence information on the White Rose Research Online record for the item. Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. -
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. -
Arxiv:0809.1275V2
How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits Guillem Anglada-Escud´e1, Mercedes L´opez-Morales1,2, John E. Chambers1 [email protected], [email protected], [email protected] ABSTRACT The Doppler technique measures the reflex radial motion of a star induced by the presence of companions and is the most successful method to detect ex- oplanets. If several planets are present, their signals will appear combined in the radial motion of the star, leading to potential misinterpretations of the data. Specifically, two planets in 2:1 resonant orbits can mimic the signal of a sin- gle planet in an eccentric orbit. We quantify the implications of this statistical degeneracy for a representative sample of the reported single exoplanets with available datasets, finding that 1) around 35% percent of the published eccentric one-planet solutions are statistically indistinguishible from planetary systems in 2:1 orbital resonance, 2) another 40% cannot be statistically distinguished from a circular orbital solution and 3) planets with masses comparable to Earth could be hidden in known orbital solutions of eccentric super-Earths and Neptune mass planets. Subject headings: Exoplanets – Orbital dynamics – Planet detection – Doppler method arXiv:0809.1275v2 [astro-ph] 25 Nov 2009 Introduction Most of the +300 exoplanets found to date have been discovered using the Doppler tech- nique, which measures the reflex motion of the host star induced by the planets (Mayor & Queloz 1995; Marcy & Butler 1996). The diverse characteristics of these exoplanets are somewhat surprising. Many of them are similar in mass to Jupiter, but orbit much closer to their 1Carnegie Institution of Washington, Department of Terrestrial Magnetism, 5241 Broad Branch Rd. -
Winter Observing Notes
Wynyard Planetarium & Observatory Winter Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Tour of the Sky with the Naked Eye NGC 457 CASSIOPEIA eta Cas Look for Notice how the constellations 5 the ‘W’ swing around Polaris during shape the night Is Dubhe yellowish compared 2 Polaris to Merak? Dubhe 3 Merak URSA MINOR Kochab 1 Is Kochab orange Pherkad compared to Polaris? THE PLOUGH 4 Mizar Alcor Figure 1: Sketch of the northern sky in winter. North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. To your right is a group of stars like the outline of a saucepan standing up on it’s handle. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The top two stars are called the Pointers. Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white-hot. 2. Use the Pointers to guide you to the left, to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the right are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. Check with binoculars. © Rob Peeling, CaDAS, 2007 version 2.0 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Polaris, Kochab and Pherkad mark the constellation Ursa Minor, the Little Bear. -
February 14, 2015 7:00Pm at the Herrett Center for Arts & Science Colleagues, College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Saturday, February 14, 2015 7:00pm at the Herrett Center for Arts & Science Colleagues, College of Southern Idaho. Public Star Party Follows at the It’s that time of year when obstacles appear in the sky. In particular, this year is Centennial Obs. loaded with fog. It got in the way of letting us see the dance of the Jovian moons late last month, and it’s hindered our views of other unique shows. Still, members Club Officers reported finding enough of a clear sky to let us see Comet Lovejoy, and some great photos by members are popping up on the Facebook page. Robert Mayer, President This month, however, is a great opportunity to see the benefit of something [email protected] getting in the way. Our own Chris Anderson of the Herrett Center has been using 208-312-1203 the Centennial Observatory’s scope to do work on occultation’s, particularly with asteroids. This month’s MVAS meeting on Feb. 14th will give him the stage to Terry Wofford, Vice President show us just how this all works. [email protected] The following weekend may also be the time the weather allows us to resume 208-308-1821 MVAS-only star parties. Feb. 21 is a great window for a possible star party; we’ll announce the location if the weather permits. However, if we don’t get that Gary Leavitt, Secretary window, we’ll fall back on what has become a MVAS tradition: Planetarium night [email protected] at the Herrett Center. -
The ELODIE Survey for Northern Extra-Solar Planets?,??,???
A&A 410, 1039–1049 (2003) Astronomy DOI: 10.1051/0004-6361:20031340 & c ESO 2003 Astrophysics The ELODIE survey for northern extra-solar planets?;??;??? I. Six new extra-solar planet candidates C. Perrier1,J.-P.Sivan2,D.Naef3,J.L.Beuzit1, M. Mayor3,D.Queloz3,andS.Udry3 1 Laboratoire d’Astrophysique de Grenoble, Universit´e J. Fourier, BP 53, 38041 Grenoble, France 2 Observatoire de Haute-Provence, 04870 St-Michel L’Observatoire, France 3 Observatoire de Gen`eve, 51 Ch. des Maillettes, 1290 Sauverny, Switzerland Received 17 July 2002 / Accepted 1 August 2003 Abstract. Precise radial-velocity observations at Haute-Provence Observatory (OHP, France) with the ELODIE echelle spec- trograph have been undertaken since 1994. In addition to several discoveries described elsewhere, including and following that of 51 Peg b, they reveal new sub-stellar companions with essentially moderate to long periods. We report here about such companions orbiting five solar-type stars (HD 8574, HD 23596, HD 33636, HD 50554, HD 106252) and one sub-giant star (HD 190228). The companion of HD 8574 has an intermediate period of 227.55 days and a semi-major axis of 0.77 AU. All other companions have long periods, exceeding 3 years, and consequently their semi-major axes are around or above 2 AU. The detected companions have minimum masses m2 sin i ranging from slightly more than 2 MJup to 10.6 MJup. These additional objects reinforce the conclusion that most planetary companions have masses lower than 5 MJup but with a tail of the mass dis- tribution going up above 15 MJup. -
Urania Nr 5/2001
Eta Carinae To zdjęcie mgławicy otaczającej gwiazdę // Carinae uzyskano za po mocą telskopu kosmicznego Hubble a (K. Davidson i J. Mors). Porównując je z innymi zdjęciami, a w szczególności z obrazem wyko nanym 17 miesięcy wcześniej, Auto rzy stwierdzili rozprężanie się mgła wicy z szybkością ok. 2,5 min km/h, co prowadzi do wniosku, że rozpo częła ona swe istnienie około 150 lat temu. To bardzo ciekawy i intrygujący wynik. Otóż największy znany roz błysk )j Carinae miał miejsce w roku 1840. Wtedy gwiazda ta stała się naj jaśniejszą gwiazdą południowego nie ba i jasność jej przez krótki czas znacznie przewyższała blask gwiaz dy Canopus. Jednak pyłowy dysk ob serwowany wokół)/ Carinae wydaje się być znacznie młodszy - jego wiek (ekspansji) jest oceniany na 100 lat, co może znaczyć, że powstał w cza sie innego, mniejszego wybuchu ob serwowanego w roku 1890. Więcej na temat tego intrygują cego obiektu przeczytać można we wnątrz numeru, w artykule poświę conym tej gwieździe. NGC 6537 Obserwacje przeprowadzone teleskopem Hubble’a pokazały istnienie wielkich falowych struktur w mgławicy Czerwonego Pająka (NGC 6537) w gwiazdozbiorze Strzelca.Ta gorąca i „wietrzna” mgławica powstała wokół jednej z najgorętszych gwiazd Wszech świata, której wiatr gwiazdowy wiejący z prędkością 2000-4500 kilometrów na sekundę wytwarza fale o wysokości 100 miliardów kilometrów. Sama mgławica rozszerza się z szybkością 300 km/s. Jest też ona wyjątkowo gorąca — ok. 10000 K. Sama gwiazda, która utworzyła mgławicę, jest obecnie białym karłem i musi mieć temperaturę nie niższą niż pół miliona stopni — jest tak gorąca, że nie widać jej w obszarach uzyskanych teleskopem Hubble’a, a świeci głównie w promieniowaniu X. -
Pos(ICRC2019)832 † ∗ [email protected] Speaker
Probing Particle Diffusion around Two Nearby Pulsars with TeV Gamma-Ray Observations from HAWC PoS(ICRC2019)832 Hao Zhou∗ Los Alamos National Laboratory E-mail: [email protected] for the HAWC Collaborationy Nearby cosmic-ray accelerators, especially pulsar wind nebulae, are possible origins of the local multi-GeV positron excess. Pulsar Geminga and B0656+14, less than 300 pc from the Earth, have been postulated as the main sources of the positron excess. With one and half years of data, the HAWC gamma-ray observatory discovered very extended TeV gamma-ray structures produced from high-energy electrons and positrons around these two nearby middle-aged pulsars. Morphology studies suggest that the diffusion in the vicinity of these two pulsars is 100 times slower than the average in our Galaxy. This result provides important constraints on the origin of positron excess, but raises questions like why diffusion is so slow at high energies near these pulsars. With more than twice of data from the previous results, we now explore the possibility of energy-dependent diffusion at these sources. 36th International Cosmic Ray Conference -ICRC2019- July 24th - August 1st, 2019 Madison, WI, U.S.A. ∗Speaker. yFor a complete author list and acknowledgemets, see PoS(ICRC2019)1177 and http://www.hawc- observatory.org/collaboration/icrc2019.php c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). http://pos.sissa.it/ Probing Particle Diffusion with HAWC Hao Zhou 1. Introduction Pulsar wind nebulae are known as efficient particle accelerators of electrons and positrons. -
Redox DAS Artist List for Period: 01.10.2017
Page: 1 Redox D.A.S. Artist List for period: 01.10.2017 - 31.10.2017 Date time: Number: Title: Artist: Publisher Lang: 01.10.2017 00:02:40 HD 60753 TWO GHOSTS HARRY STYLES ANG 01.10.2017 00:06:22 HD 05631 BANKS OF THE OHIO OLIVIA NEWTON JOHN ANG 01.10.2017 00:09:34 HD 60294 BITE MY TONGUE THE BEACH ANG 01.10.2017 00:13:16 HD 26897 BORN TO RUN SUZY QUATRO ANG 01.10.2017 00:18:12 HD 56309 CIAO CIAO KATARINA MALA SLO 01.10.2017 00:20:55 HD 34821 OCEAN DRIVE LIGHTHOUSE FAMILY ANG 01.10.2017 00:24:41 HD 08562 NISEM JAZ SLAVKO IVANCIC SLO 01.10.2017 00:28:29 HD 59945 LEPE BESEDE PROTEUS SLO 01.10.2017 00:31:20 HD 03206 BLAME IT ON THE WEATHERMAN B WITCHED ANG 01.10.2017 00:34:52 HD 16013 OD TU NAPREJ NAVDIH TABU SLO 01.10.2017 00:38:14 HD 06982 I´M EVERY WOMAN WHITNEY HOUSTON ANG 01.10.2017 00:43:05 HD 05890 CRAZY LITTLE THING CALLED LOVE QUEEN ANG 01.10.2017 00:45:37 HD 57523 WHEN I WAS A BOY JEFF LYNNE (ELO) ANG 01.10.2017 00:48:46 HD 60269 MESTO (FEAT. VESNA ZORNIK) BREST SLO 01.10.2017 00:52:21 HD 06008 DEEPLY DIPPY RIGHT SAID FRED ANG 01.10.2017 00:55:35 HD 06012 UNCHAINED MELODY RIGHTEOUS BROTHERS ANG 01.10.2017 00:59:10 HD 60959 OKNA ORLEK SLO 01.10.2017 01:03:56 HD 59941 SAY SOMETHING LOVING THE XX ANG 01.10.2017 01:07:51 HD 15174 REAL GOOD LOOKING BOY THE WHO ANG 01.10.2017 01:13:37 HD 59654 RECI MI DA MANOUCHE SLO 01.10.2017 01:16:47 HD 60502 SE PREPOZNAS SHEBY SLO 01.10.2017 01:20:35 HD 06413 MARGUERITA TIME STATUS QUO ANG 01.10.2017 01:23:52 HD 06388 MAMA SPICE GIRLS ANG 01.10.2017 01:27:25 HD 02680 HIGHER GROUND ERIC CLAPTON ANG 01.10.2017 01:31:20 HD 59929 NE POZABI, DA SI LEPA LUKA SESEK & PROPER SLO 01.10.2017 01:34:57 HD 02131 BONNIE & CLYDE JAY-Z FEAT. -
Atlas Menor Was Objects to Slowly Change Over Time
C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts. -
Gemini Deutscher Name: Zwillinge Gem Atlas (2000.0)
Lateinischer Name: Deutscher Name: Gem Gemini Zwillinge Atlas (2000.0) Karte Cambridge Star Kulmination um 3, 9 Atlas Mitternacht: Benachbarte 5, 6, 11, Sky Atlas Sternbilder: 12 Aur Cnc CMi Lyn 4. Januar Mon Ori Tau Deklinationsbereich: 10° ... 35° Fläche am Himmel: 514° 2 Mythologie und Geschichte: Castor und Pollux waren schon in vielen Kulturen als Zwillinge bekannt. Manchmal wurden sie auch Die Dioscuri oder die Söhne des Zeus, des Königs der Götter bezeichnet. Ihre Mutter war die wunderschöne Leda, der Zeus in der Gestalt eines Schwans erschien. Pollux besaß eine unsterbliche Seele; bei seinem Tode war ihm ein Zuhause auf dem Olymp zugesprochen. Castor jedoch war sterblich. Einige sagten, Castors Vater wäre nicht der mächtige Zeus gewesen, sondern der irdische König Tyndareos von Sparta. Somit war Castor, wie auch der übrigen Menschheit, die Unterwelt von Hades als allerletzte Ruhestätte bestimmt. Diese Welt des Todes war kein Platz der Bestrafung wie in der christlichen Vorstellung, sondern ein Platz unablässiger Teilnahmslosigkeit und Langeweile. Castor zeichnete sich in der Reitkunst aus, während sich Pollux im Boxen und im Kämpfen von Schlachten bewährte. Man erzählte sich, die beiden wären sich so ähnlich, wie es nur Zwillinge sein könnten. Beide heirateten die hübschen Töchter eines Königs von Sparta. Ein trauriger Tag kam, als während eines Aufruhrs eine Lanze Castors Herz durchbohrte. Pollux begriff, dass nun sein Zwillingsbruder für immer im Hades verweilen würde. Er bat Zeus, ihn zusammen mit ihm in die Unterwelt zu senden. Zeus war aber nicht fähig diese Bitte zu gewähren. Er versprach jedoch Pollux, dass er und sein Bruder Castor die Hälfte ihrer Zeit auf dem Olymp und die andere Hälfte im Hades, verbringen würden.