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List of Easy Double Stars for Winter and Spring = Easy = Not Too Difficult = Difficult but Possible
List of Easy Double Stars for Winter and Spring = easy = not too difficult = difficult but possible 1. Sigma Cassiopeiae (STF 3049). 23 hr 59.0 min +55 deg 45 min This system is tight but very beautiful. Use a high magnification (150x or more). Primary: 5.2, yellow or white Seconary: 7.2 (3.0″), blue 2. Eta Cassiopeiae (Achird, STF 60). 00 hr 49.1 min +57 deg 49 min This is a multiple system with many stars, but I will restrict myself to the brightest one here. Primary: 3.5, yellow. Secondary: 7.4 (13.2″), purple or brown 3. 65 Piscium (STF 61). 00 hr 49.9 min +27 deg 43 min Primary: 6.3, yellow Secondary: 6.3 (4.1″), yellow 4. Psi-1 Piscium (STF 88). 01 hr 05.7 min +21 deg 28 min This double forms a T-shaped asterism with Psi-2, Psi-3 and Chi Piscium. Psi-1 is the uppermost of the four. Primary: 5.3, yellow or white Secondary: 5.5 (29.7), yellow or white 5. Zeta Piscium (STF 100). 01 hr 13.7 min +07 deg 35 min Primary: 5.2, white or yellow Secondary: 6.3, white or lilac (or blue) 6. Gamma Arietis (Mesarthim, STF 180). 01 hr 53.5 min +19 deg 18 min “The Ram’s Eyes” Primary: 4.5, white Secondary: 4.6 (7.5″), white 7. Lambda Arietis (H 5 12). 01 hr 57.9 min +23 deg 36 min Primary: 4.8, white or yellow Secondary: 6.7 (37.1″), silver-white or blue 8. -
Arxiv:2006.10868V2 [Astro-Ph.SR] 9 Apr 2021 Spain and Institut D’Estudis Espacials De Catalunya (IEEC), C/Gran Capit`A2-4, E-08034 2 Serenelli, Weiss, Aerts Et Al
Noname manuscript No. (will be inserted by the editor) Weighing stars from birth to death: mass determination methods across the HRD Aldo Serenelli · Achim Weiss · Conny Aerts · George C. Angelou · David Baroch · Nate Bastian · Paul G. Beck · Maria Bergemann · Joachim M. Bestenlehner · Ian Czekala · Nancy Elias-Rosa · Ana Escorza · Vincent Van Eylen · Diane K. Feuillet · Davide Gandolfi · Mark Gieles · L´eoGirardi · Yveline Lebreton · Nicolas Lodieu · Marie Martig · Marcelo M. Miller Bertolami · Joey S.G. Mombarg · Juan Carlos Morales · Andr´esMoya · Benard Nsamba · KreˇsimirPavlovski · May G. Pedersen · Ignasi Ribas · Fabian R.N. Schneider · Victor Silva Aguirre · Keivan G. Stassun · Eline Tolstoy · Pier-Emmanuel Tremblay · Konstanze Zwintz Received: date / Accepted: date A. Serenelli Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E- 08193, Spain and Institut d'Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2, Barcelona, E-08034, Spain E-mail: [email protected] A. Weiss Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany C. Aerts Institute of Astronomy, Department of Physics & Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium and Department of Astrophysics, IMAPP, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, the Netherlands G.C. Angelou Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany D. Baroch J. C. Morales I. Ribas Institute of· Space Sciences· (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E-08193, arXiv:2006.10868v2 [astro-ph.SR] 9 Apr 2021 Spain and Institut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capit`a2-4, E-08034 2 Serenelli, Weiss, Aerts et al. -
The Evening Sky Map
I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O p l f e i n h d o P t O o N ) l h a r g Z i u s , o I l C t P h R I r e o R N ( O o r C r H e t L p h p E E i s t D H a ( r g T F i . O B NORTH D R e N M h t E A X O e s A H U M C T . I P N S L E E P Z “ E A N H O NORTHERN HEMISPHERE M T R T Y N H E ” K E η ) W S . T T E W U B R N W D E T T W T H h A The Evening Sky Map e MAY 2021 E . C ) Cluster O N FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY r S L a o K e Double r Y E t B h R M t e PERSEUS A a A r CASSIOPEIA n e S SKY MAP SHOWS HOW Get Sky Calendar on Twitter P δ r T C G C A CEPHEUS r E o R e J s O h Sky Calendar – May 2021 http://twitter.com/skymaps M39 s B THE NIGHT SKY LOOKS T U ( O i N s r L D o a j A NE I I a μ p T EARLY MAY PM T 10 r 61 M S o S 3 Last Quarter Moon at 19:51 UT. -
Lunar Mansion Names in South-West China
Onoma 51 Journal of the International Council of Onomastic Sciences ISSN: 0078-463X; e-ISSN: 1783-1644 Journal homepage: https://onomajournal.org/ Lunar mansion names in South-West China: An etymological reconstruction of ancestral astronomical designations in Moso, Pumi, and Yi cultures compared with Chinese and Tibetan contexts DOI: 10.34158/ONOMA.51/2016/6 Xu Duoduo National University of Singapore (NUS), Asia Research Institute (ARI), Singapore [email protected] To cite this article: Xu Duoduo. 2016. Lunar mansion names in South-West China: An etymological reconstruction of ancestral astronomical designations in Moso, Pumi, and Yi cultures compared with Chinese and Tibetan contexts. Onoma 51, 113–143. DOI: 10.34158/ONOMA.51/2016/6 To link to this article: https://doi.org/10.34158/ONOMA.51/2016/6 © Onoma and the author. Lunar mansion names in South-West China: An etymological reconstruction of ancestral astronomical designations in Moso, Pumi, and Yi cultures compared with Chinese and Tibetan contexts Abstract: The present study aims at an etymological reconstruction of lunar mansion designations of the Moso, Pumi, and Yi people from South-West China. Those lunar mansions are generally named after animals. A systematic examination on these astronomical names reveals frequent borrowing processes among these cultures, extended to Tibetan and Chinese contexts. Three patterns of direct borrowing of the lunar mansion names can be highlighted in addition to compatible morphological structures in some designation. This comparative research also provides innovative 114 XU DUODUO solutions to several issues still unsolved from the current studies on lunar mansions focused on specific ethnic groups. -
Korotangi (The Dove)
Korotangi (The Dove) The legend of the korotangi is that it came in the Tainui waka as one of the heirlooms which had been blessed by the high priests in Hawaiiki and which in the new country, would ensure good hunting for the tribe. It was said that the Kawhia and Waikato tribes, who descended from Tainui stock, took the korotangi into battle with them, setting it up on a hill and consulting it as an oracle. The "korotangi" can mean "to roar and rush as the sound of water" in either Maori, Hawaiian or Samoan has been used to support the legend that it was bought on the Tainui waka from afar. The expression “Korotangi” is still used as a term of endearment, or as a simile for any object treasured or loved. A mother lamenting the death of a child will, in her lament, refer to her lost one as her “Korotangi.” 1 No doubt the simile has its origin in the above tradition, which also seems to be a fea- sible explanation of the waiata. It certainly explains the reference to the eat- ing of the pohata leaves and the huahua from Rotorua, as well as the allu- sion to the taumata (hill-top or ridge). The Korotangi, Tawhio Throne, and the art work depicting The Lost Child TeManawa and Korotangi, arrived at Turangawaewae Marae on the same day. The Heart of Heaven is in part the sharing of the walk of TeManawa who lives these things, has fulfilled prophesy. Her journey has been documented since 1992 to current. -
Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem
Informazioni su questo libro Si tratta della copia digitale di un libro che per generazioni è stato conservata negli scaffali di una biblioteca prima di essere digitalizzato da Google nell’ambito del progetto volto a rendere disponibili online i libri di tutto il mondo. Ha sopravvissuto abbastanza per non essere più protetto dai diritti di copyright e diventare di pubblico dominio. Un libro di pubblico dominio è un libro che non è mai stato protetto dal copyright o i cui termini legali di copyright sono scaduti. La classificazione di un libro come di pubblico dominio può variare da paese a paese. I libri di pubblico dominio sono l’anello di congiunzione con il passato, rappresentano un patrimonio storico, culturale e di conoscenza spesso difficile da scoprire. Commenti, note e altre annotazioni a margine presenti nel volume originale compariranno in questo file, come testimonianza del lungo viaggio percorso dal libro, dall’editore originale alla biblioteca, per giungere fino a te. Linee guide per l’utilizzo Google è orgoglioso di essere il partner delle biblioteche per digitalizzare i materiali di pubblico dominio e renderli universalmente disponibili. I libri di pubblico dominio appartengono al pubblico e noi ne siamo solamente i custodi. Tuttavia questo lavoro è oneroso, pertanto, per poter continuare ad offrire questo servizio abbiamo preso alcune iniziative per impedire l’utilizzo illecito da parte di soggetti commerciali, compresa l’imposizione di restrizioni sull’invio di query automatizzate. Inoltre ti chiediamo di: + Non fare un uso commerciale di questi file Abbiamo concepito Google Ricerca Libri per l’uso da parte dei singoli utenti privati e ti chiediamo di utilizzare questi file per uso personale e non a fini commerciali. -
Reduced Maximum Mass-Loss Rate of OH/IR Stars Due to Overlooked Binary Interaction
The University of Manchester Research Reduced maximum mass-loss rate of OH/IR stars due to overlooked binary interaction DOI: 10.1038/s41550-019-0703-5 Document Version Accepted author manuscript Link to publication record in Manchester Research Explorer Citation for published version (APA): Decin, L., Homan, W., Danilovich, T., de Koter, A., Engels, D., Waters, L. B. F. M., Muller, S., Gielen, C., Garca- Hernandez, D. A., Stancliffe, R., Van de Sande, M., Molenberghs, G., Kerschbaum, F., Zijlstra, A., & El Mellah, I. (2019). Reduced maximum mass-loss rate of OH/IR stars due to overlooked binary interaction. Nature Astronomy, 3(5), 408-415. https://doi.org/10.1038/s41550-019-0703-5 Published in: Nature Astronomy Citing this paper Please note that where the full-text provided on Manchester Research Explorer is the Author Accepted Manuscript or Proof version this may differ from the final Published version. If citing, it is advised that you check and use the publisher's definitive version. General rights Copyright and moral rights for the publications made accessible in the Research Explorer are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Takedown policy If you believe that this document breaches copyright please refer to the University of Manchester’s Takedown Procedures [http://man.ac.uk/04Y6Bo] or contact [email protected] providing relevant details, so we can investigate your claim. Download date:08. Oct. 2021 Reduced maximum mass-loss rate of OH/IR stars due to overlooked binary interaction L. -
Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem
Informazioni su questo libro Si tratta della copia digitale di un libro che per generazioni è stato conservata negli scaffali di una biblioteca prima di essere digitalizzato da Google nell’ambito del progetto volto a rendere disponibili online i libri di tutto il mondo. Ha sopravvissuto abbastanza per non essere più protetto dai diritti di copyright e diventare di pubblico dominio. Un libro di pubblico dominio è un libro che non è mai stato protetto dal copyright o i cui termini legali di copyright sono scaduti. La classificazione di un libro come di pubblico dominio può variare da paese a paese. I libri di pubblico dominio sono l’anello di congiunzione con il passato, rappresentano un patrimonio storico, culturale e di conoscenza spesso difficile da scoprire. Commenti, note e altre annotazioni a margine presenti nel volume originale compariranno in questo file, come testimonianza del lungo viaggio percorso dal libro, dall’editore originale alla biblioteca, per giungere fino a te. Linee guide per l’utilizzo Google è orgoglioso di essere il partner delle biblioteche per digitalizzare i materiali di pubblico dominio e renderli universalmente disponibili. I libri di pubblico dominio appartengono al pubblico e noi ne siamo solamente i custodi. Tuttavia questo lavoro è oneroso, pertanto, per poter continuare ad offrire questo servizio abbiamo preso alcune iniziative per impedire l’utilizzo illecito da parte di soggetti commerciali, compresa l’imposizione di restrizioni sull’invio di query automatizzate. Inoltre ti chiediamo di: + Non fare un uso commerciale di questi file Abbiamo concepito Google Ricerca Libri per l’uso da parte dei singoli utenti privati e ti chiediamo di utilizzare questi file per uso personale e non a fini commerciali. -
Starry Nights Typeset
Index Antares 104,106-107 Anubis 28 Apollo 53,119,130,136 21-centimeter radiation 206 apparent magnitude 7,156-157,177,223 57 Cygni 140 Aquarius 146,160-161,164 61 Cygni 139,142 Aquila 128,131,146-149 3C 9 (quasar) 180 Arcas 78 3C 48 (quasar) 90 Archer 119 3C 273 (quasar) 89-90 arctic circle 103,175,212 absorption spectrum 25 Arcturus 17,79,93-96,98-100 Acadia 78 Ariadne 101 Achernar 67-68,162,217 Aries 167,183,196,217 Acubens (star in Cancer) 39 Arrow 149 Adhara (star in Canis Major) 22,67 Ascella (star in Sagittarius) 120 Aesculapius 115 asterisms 130 Age of Aquarius 161 astrology 161,196 age of clusters 186 Atlantis 140 age of stars 114 Atlas 14 Age of the Fish 196 Auriga 17 Al Rischa (star in Pisces) 196 autumnal equinox 174,223 Al Tarf (star in Cancer) 39 azimuth 171,223 Al- (prefix in star names) 4 Bacchus 101 Albireo (star in Cygnus) 144 Barnard’s Star 64-65,116 Alcmene 52,112 Barnard, E. 116 Alcor (star in Big Dipper) 14,78,82 barred spiral galaxies 179 Alcyone (star in Pleiades) 14 Bayer, Johan 125 Aldebaran 11,15,22,24 Becvar, A. 221 Alderamin (star in Cepheus) 154 Beehive (M 44) 42-43,45,50 Alexandria 7 Bellatrix (star in Orion) 9,107 Alfirk (star in Cepheus) 154 Algedi (star in Capricornus) 159 Berenice 70 Algeiba (star in Leo) 59,61 Bessel, Friedrich W. 27,142 Algenib (star in Pegasus) 167 Beta Cassiopeia 169 Algol (star in Perseus) 204-205,210 Beta Centauri 162,176 Alhena (star in Gemini) 32 Beta Crucis 162 Alioth (star in Big Dipper) 78 Beta Lyrae 132-133 Alkaid (star in Big Dipper) 78,80 Betelgeuse 10,22,24 Almagest 39 big -
Sky High 2008 28Nov Completed.Pub
Sky-High 2008 Solar Prominences, 19th July 2007 The 16th annual guide to astronomical phenomena visible from Ireland during the year ahead (naked-eye, binocular and beyond) By Liam Smyth and John O’Neill Published by the Irish Astronomical Society € 5 P.O. Box 2547, Dublin 14. e-mail: [email protected] www.irishastrosoc.org Page 1 Foreword Contents 3 Your Night Sky Primer We send greetings to all fellow astronomers and 5 Sky Diary 2008 welcome them to this, the sixteenth edition of Sky-High. 8 Phases of Moon; Sunrise and Sunset in 2008 We thank the following contributors for their 9 The Planets in 2008 articles: Patricia Carroll, John Flannery and James 11 Eclipses in 2008 O’Connor. The remaining material was written by the editors John O’Neill and Liam Smyth. The Gal- 13 Comets in 2008 lery has images and drawings by Society members. 15 Meteors Showers in 2008 The times of sunrise etc. are from SUNRISE and 17 Asteroids in 2008 double star diagrams are from BINARY, both by J. O’Neill. 19 Variable Stars in 2008 We are always glad to hear what you liked, or 20 More Favourite Double Stars what you would like to have included in Sky-High. 23 From Eros to Apophis – a Century of Near Earth If we have slipped up on any matter of fact, let us Asteroids know. We can put a correction in future issues. 25 Spaceflight in 2008 And if you have any problem with understanding the contents or would like more information on 28 Gallery any topic, feel free to contact us at the Society e- mail address [email protected]. -
Discovery of a Shell of Neutral Atomic Hydrogen Surrounding the Carbon Star IRC+10216
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 6 February 2015 (MN LATEX style file v2.2) Discovery of a Shell of Neutral Atomic Hydrogen Surrounding the Carbon Star IRC+10216 L. D. Matthews1, E. G´erard2, T. Le Bertre3 1Massachusetts Institute of Technology Haystack Observatory, Off Route 40, Westford, MA 01886 USA 2GEPI, UMR 8111, Observatoire de Paris, 5 Place J. Janssen, F-92195 Meudon Cedex, France 3LERMA, UMR 8112, Observatoire de Paris, 61 av. de l’Observatoire, F-75014 Paris, France 6 February 2015 ABSTRACT We have used the Robert C. Byrd Green Bank Telescope to perform the most sensitive search to date for neutral atomic hydrogen (H i) in the circumstellar envelope (CSE) of the carbon star IRC+10216. Our observations have uncovered a low surface brightness H i shell of diameter ∼ 1300′′ (∼0.8 pc), centered on IRC+10216. The H i shell has an angular extent comparable to the far ultraviolet-emitting astrosphere of IRC+10216 previously detected with the GALEX satellite, and its kinematics are consistent with circumstellar matter that has been decelerated by the local interstellar medium. The shell appears to completely surround the star, but the highest H i column densities are measured along the leading edge of the shell, near the location of a previously identified bow shock. We estimate a total mass of atomic hydrogen associated with −3 IRC+10216 CSE of MHI ∼ 3 × 10 M⊙. This is only a small fraction of the expected total mass of the CSE (<1%) and is consistent with the bulk of the stellar wind originating in molecular rather than atomic form, as expected for a cool star with ◦ ◦ an effective temperature Teff ∼<2200 K. -
Extrasolar Planets and Their Host Stars
Kaspar von Braun & Tabetha S. Boyajian Extrasolar Planets and Their Host Stars July 25, 2017 arXiv:1707.07405v1 [astro-ph.EP] 24 Jul 2017 Springer Preface In astronomy or indeed any collaborative environment, it pays to figure out with whom one can work well. From existing projects or simply conversations, research ideas appear, are developed, take shape, sometimes take a detour into some un- expected directions, often need to be refocused, are sometimes divided up and/or distributed among collaborators, and are (hopefully) published. After a number of these cycles repeat, something bigger may be born, all of which one then tries to simultaneously fit into one’s head for what feels like a challenging amount of time. That was certainly the case a long time ago when writing a PhD dissertation. Since then, there have been postdoctoral fellowships and appointments, permanent and adjunct positions, and former, current, and future collaborators. And yet, con- versations spawn research ideas, which take many different turns and may divide up into a multitude of approaches or related or perhaps unrelated subjects. Again, one had better figure out with whom one likes to work. And again, in the process of writing this Brief, one needs create something bigger by focusing the relevant pieces of work into one (hopefully) coherent manuscript. It is an honor, a privi- lege, an amazing experience, and simply a lot of fun to be and have been working with all the people who have had an influence on our work and thereby on this book. To quote the late and great Jim Croce: ”If you dig it, do it.