Objekti Globoko V Vesolju Oktobra Je Posnel Hubblov Teleskop

Total Page:16

File Type:pdf, Size:1020Kb

Objekti Globoko V Vesolju Oktobra Je Posnel Hubblov Teleskop Interno glasilo Astronomskega druˇstva Javornik Stevilkaˇ 152, Letnik XIII, September 2012 www: http://www.adj.si, email: [email protected] ISSN 1581-1379 Objekti globoko v vesolju oktobra je posnel Hubblov teleskop. V resnici smo videli nekaj, ˇcesarHubble ne pokaˇze: tam, kjer je Hubblova slika V zaˇcetkuoktobra nastopi astronomska tema ob 20:21 preˇzgana,smo videli, kako se jedro boˇcinad ozadjem in traja 9:01 ur, na koncu se zaˇcneob 18:30 in traja starih zvezd na prehodu iz jedra v spiralna kraka, po skoraj deset ur in pol. Astronomski mrak v tem mesecu krakih pa so bile zelo lepo videti kopice pravkar rojenih traja 35 minut. Ko se znoˇci,so poletna ozvezdja ˇse zvezd safirne barve in seveda ˇstevilne porodniˇsnice vedno na nebu, do jutra pa vzidejo zimska. zvezd, ki so bile videti kot rubini, rjavkasti oblaki Oktobra opolnoˇcikulminirajo ozvezdja Kasiopeja medzveznega prahu pa so se z ukrivljenimi koniˇcastimi z razsutimi kopicami NGC 129*, NGC 457*, NGC jeziki zajedali daleˇcv jedro. 205, M 103 (NGC 581), NGC 663*, Collinder 463*, Stock 2*, Markarian 6*, Melotte 15*, Trumpler 3*, M 52 (NGC 7654) in NGC 7789*, Andromeda z galak- Trikotnik sijo M 31* (NGC 224) s spremljevalkama M 32* (NGC 221) in M 110 (NGC 205), razsuto kopico NGC 752* in Tudi M33 je ˇclanicalokalne jate, oddaljena tri mili- planetarno meglico NGC 7662*, Trikotniku z galak- jone svetlobnih let. Je najmanjˇsamed tremi velikimi, sijo M33 (NGC 598), Ribi z galaksijo M74 (NGC 628), vidimo jo zvrha, a ker je blizu, jo s temnega opa- Kit z galaksijo M77* (NGC 1068) in Kipar z galaksijo zovaliˇsˇcaopazimo tudi s prostimi oˇcmi,ˇceprav njen NGC 253. Rimska cesta se boˇciˇceznebo od vzhoda povrˇsinskisij ni velik. Binokular in manjˇsiteleskop ˇze do zahoda in je ˇsevedno v ugodni legi za opazovanje z pokaˇzetanjen obris, dober ogled nudi teleskop z ob- binokularjem. Zvezdica oznaˇcujeobjekte, ki se jih da jektivom 25 cm ali veˇc.Pri emisijski meglici NGC 604 opazovati z opazovaliˇsˇc,kjer nebo ni temno. na vrhu njenega severnega kraka si lahko pomagamo s filtrom za meglice, ki bo poveˇcalkontrast s tem, da bo Kasiopeja priduˇsilsvetlobo zvezd. NGC 129, razsuta kopica, je s temnega opazovaliˇsˇca opazna celo sprostimi oˇcmi,v binokularju je videti kot Ribi majhen trikotnik zvezd, v teleskopu pa se prikaˇzeprecej ˇsibkejˇsih,ki iz trikotnika uhajajo proti severu. NGC Galaksija M74 (NGC 628) ima na videz zelo ma- 457 se je splaˇcapogledati skozi teleskop: ovalna je in jhno jedro: v majhnih daljnogledih ga komaj loˇcimo dve svetli zvezdi, ki sicer nista ˇclanicirazsute kopice, od zvezde, a ˇze objektiv premera 10 cm v ugod- svetita kot oˇcisove, zato jo Anglosasi imenujejo Kopica nih razmerah daje slutiti spiralno zgradbo, s 40 cm sova. pa v jasno vidnih spiralnih krakih lepo loˇcimo vozle svetlejˇsihsvezd in zvezdne oblake v tej galaksiji. V Andromeda resnici je 55 milijonov svetlobnih let daleˇcin ima pre- mer 95 tisoˇcsvetlobnih let. Jedro je majhno, a svetlo, Najsvetlejˇsagalaksija (ˇcene ˇstejemonaˇseGalaksije), sama galaksija pa je lepo simetriˇcna. kar jih vidimo, je Andromedina meglica, ˇclanicalokalne jate, ki je oddaljena 2,5 milijona svetlobnih let. Ni jasno, ali je veˇcjaod naˇseGalaksije ali ne, in tudi ne, Kit ali ima tako kot naˇsa preˇcko ali ne, ima pa dvojno jedro, kar je najbrˇzposledica tega, da okoli njene ˇcrne Spiralna galaksija M77 (NGC 1068) je 60 milijonov luknje kroˇziprecjˇsnjaskupina zvezd v nasprotni smeri, svetlobnih let daleˇc,svetlejˇsidel, bogat z mladimi zvez- kot ostale. Je pa ˇzejasno, da je verjetnost 41%, da dami, ima premer 120, ˇsibkejˇsi,v katerem moˇcno pre- bosta ti dve galaksiji ˇcelnotrˇciliˇcez 4 miljarde let in vladujejo starejˇsezvezde, pa 170 tisoˇcsvetlobnih let. bosta 2 miljardi let kasneje ˇzezliti v veliko eliptiˇcno Svetlejˇsidel ima maso 27 milijard sonc, celotna galak- galaksijo. Verjetnost, da se zgreˇsitaje 7%, malo veˇcja, sija pa bilijon. Iz jedra beˇzijoplini s hitrostjo nekaj sto 9%, pa je, da bo z naˇsogalaksijo prej trˇcilaM 33. kilometrov na sekundo in oddajajo spekter, ki spom- A do takrat, kadar je ozraˇcjeres izjemo prozorno, inja na tistega, ki ga oddajajo planetarne meglice, kar nam nudi pogled, ki smo ga doˇziveli vsi udeleˇzenci to galaksijo uvrˇsˇcamed Seifertove galaksije. Jedro je tabora Kavka 2005: v binokularju 20×100 slika ni za- moˇcanvir radijskega in infrardeˇcegasevanja, kar si ostajala ne po barvah, ne po podrobnostih za tisto, ki jo lahko razlagamo s tem, da tam deluje majhen kvazar. VABILO Vabimo vas na meseˇcnisestanek, ki bo v torek 18. 09. 2012 ob 18h v predavalnici F4 Fakultete za matematiko in fiziko, Jadranska 19, v Ljubljani. Na meseˇcnemsestanku nam bo Rok Vidmar predstavil zanimivosti noˇcneganeba v tekoˇcemin prihodnjem mesecu. Nato se bomo dogovorili za meseˇcnodruˇstveno opazovanje, ki ga bomo izvedli v okolici Ljubljane. Vsi ˇclanidruˇstva ste vabljeni, da se nam pridruˇzite.V kolikor bi se radi udeleˇziliopazovanja, pa vas ne bo na sestanku, mi to prosim sporoˇcitepo e-poˇstina naslov [email protected]. Vabljeni! Bernard Kipar ? Uran je v zaˇcetkuoktobra na nebu vso noˇc,nato pa zahaja vse bolj zgodaj in konec meseca zaide Galaksija NGC 253 sodi med najsvetlejˇsena naˇsem okoli petih zjutraj. Nahaja se v ozvezdju Rib. nebu. Od nas je, skupaj z ostalimi ˇclanicami jate v tem ozvezdju, oddaljena 8 milijonov svetlobnih let, v Ostalo: njej je izjemno veliko medzvezdnega prahu in zvezde v ? V noˇcis 27. na 28. oktober premaknemo ure za njej nastajajo s tako vrtoglavo hitrostjo, da se v njenem eno uro nazaj. centru utegne narediti dovolj velika ˇcrnaluknja, da bo UrˇskaPajer sproˇzilakvazar. Rok Vidmar E-poˇstni seznam slo-astro Efemeride oktober 2012 Slovenski amaterski astronomi komuniciramo tudi preko poˇstnegaseznama (\mailing liste") slo-astro, (Efemeride si lahko ogledate tudi v reviji Zivljenjeˇ in tehnika.) kjer si izmenjujemo prispevke vseh vrst: opozo- Sonce Luna rila o zanimivih astronomskih dogodkih in prired- datum vzhod zahod vzhod zahod ˇcas itvah, vabila na opazovanja, poroˇcila o opazovan- 01.10. 07:01 18:42 19:01 08:21 CEST jih, vpraˇsanja, ponudbo rabljene opreme itd. Pri- 05.10. 07:06 18:34 21:27 12:15 CEST javi se lahko vsak, dodatne informacije in prijava na 10.10. 07:12 18:25 01:15 15:32 CEST http://www.adj.si/slo-astro. Trenutno ima lista 15.10. 07:19 18:15 07:12 18:00 CEST 114 ˇclanov. 20.10. 07:26 18:07 12:58 22:24 CEST Aram Karaliˇc 25.10. 07:33 17:58 15:46 02:59 CEST 30.10. 06:40 16:50 17:05 07:14 CET Planeti: ? Merkur oktobra ni viden. Objavite prispevek! ? Venera sprva vzhaja okoli pol ˇstirihzjutraj, nato Meseˇcnik potrebuje prispevke. Zato pozivam vse, pa vse kasneje in konec meseca vzide ob pol petih. ki ˇzelite kaj objaviti, da mi po elektronski poˇsti Sredi meseca se iz ozvezdja Leva preseli v ozvezdje poˇsljetesvoj prispevek. Prispevki so lahko raznovrstni: Device. poroˇciloo opazovanju, slika, risba, zanimiva astronom- ? Mars je viden zveˇcer,ko zahaja slabi dve uri za ska novica, predstavitev domaˇcega observatorija ali Soncem. V zaˇcetkumeseca se iz ozvezdja Tehtnice teleskopa, skratka { karkoli astronomskega. ˇ preseli v ozvezdje Skorpijona. Aram Karaliˇc ? Jupiter v ozvezdju Bika sprva vzhaja okoli pol desetih, nato pa vse bolj zgodaj in je konec meseca JavorniˇskiMeseˇcnikizdaja Astronomsko druˇstvo Javornik, Ljubl- na nebu ˇzeob pol osmih. jana / ISSN 1581-1379 / urednik Aram Karaliˇc / izhaja v prvi ? Saturn morda v ozvezdju Device ˇseujamemo v polovici meseca / prejemajo ga brezplaˇcno vsi ˇclaniAstronomskega druˇstva Javornik / prispevke poˇsljitena naslov [email protected] / ROK zaˇcetkumeseca, ko zahaja slabo uro za Soncem, ZA ODDAJO PRISPEVKOV JE 7. DAN V MESECU / potem pa ni veˇcviden. prispevkov praviloma ne lektoriramo / stavljeno v LATEXu.
Recommended publications
  • 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.
    [Show full text]
  • Astronomy Astrophysics
    A&A 468, 151–161 (2007) Astronomy DOI: 10.1051/0004-6361:20077073 & c ESO 2007 Astrophysics Towards absolute scales for the radii and masses of open clusters A. E. Piskunov1,2,3, E. Schilbach1, N. V. Kharchenko1,3,4, S. Röser1, and R.-D. Scholz3 1 Astronomisches Rechen-Institut, Mönchhofstraße 12-14, 69120 Heidelberg, Germany e-mail: [apiskunov;elena;nkhar;roeser]@ari.uni-heidelberg.de 2 Institute of Astronomy of the Russian Acad. Sci., 48 Pyatnitskaya Str., 109017 Moscow, Russia e-mail: [email protected] 3 Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany e-mail: [apiskunov;nkharchenko;rdscholz]@aip.de 4 Main Astronomical Observatory, 27 Academica Zabolotnogo Str., 03680 Kiev, Ukraine e-mail: [email protected] Received 10 January 2007 / Accepted 19 February 2007 ABSTRACT Aims. In this paper we derive tidal radii and masses of open clusters in the nearest kiloparsecs around the Sun. Methods. For each cluster, the mass is estimated from tidal radii determined from a fitting of three-parameter King profiles to the observed integrated density distribution. Different samples of members are investigated. Results. For 236 open clusters, all contained in the catalogue ASCC-2.5, we obtain core and tidal radii, as well as tidal masses. The distributions of the core and tidal radii peak at about 1.5 pc and 7–10 pc, respectively. A typical relative error of the core radius lies between 15% and 50%, whereas, for the majority of clusters, the tidal radius was determined with a relative accuracy better than 20%. Most of the clusters have tidal masses between 50 and 1000 m, and for about half of the clusters, the masses were obtained with a relative error better than 50%.
    [Show full text]
  • Open Clusters in Gaia
    Sede Amministrativa: Università degli Studi di Padova Dipartimento di Fisica e Astronomia “G. Galilei” Corso di Dottorato di Ricerca in Astronomia Ciclo XXX OPEN CLUSTERS IN GAIA ERA Coordinatore: Ch.mo Prof. Giampaolo Piotto Supervisore: Dr.ssa Antonella Vallenari Dottorando: Francesco Pensabene i Abstract Context. Open clusters (OCs) are optimal tracers of the Milky Way disc. They are observed at every distance from the Galactic center and their ages cover the entire lifespan of the disc. The actual OC census contain more than 3000 objects, but suffers of incom- pleteness out of the solar neighborhood and of large inhomogeneity in the parameter deter- minations present in literature. Both these aspects will be improved by the on-going space mission Gaia . In the next years Gaia will produce the most precise three-dimensional map of the Milky Way by surveying other than 1 billion of stars. For those stars Gaia will provide extremely precise measure- ment of proper motions, parallaxes and brightness. Aims. In this framework we plan to take advantage of the first Gaia data release, while preparing for the coming ones, to: i) move the first steps towards building a homogeneous data base of OCs with the high quality Gaia astrometry and photometry; ii) build, improve and test tools for the analysis of large sample of OCs; iii) use the OCs to explore the prop- erties of the disc in the solar neighborhood. Methods and Data. Using ESO archive data, we analyze the photometry and derive physical parameters, comparing data with synthetic populations and luminosity functions, of three clusters namely NGC 2225, NGC 6134 and NGC 2243.
    [Show full text]
  • Characterising Open Clusters in the Solar Neighbourhood with the Tycho-Gaia Astrometric Solution? T
    A&A 615, A49 (2018) Astronomy https://doi.org/10.1051/0004-6361/201731251 & © ESO 2018 Astrophysics Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution? T. Cantat-Gaudin1, A. Vallenari1, R. Sordo1, F. Pensabene1,2, A. Krone-Martins3, A. Moitinho3, C. Jordi4, L. Casamiquela4, L. Balaguer-Núnez4, C. Soubiran5, and N. Brouillet5 1 INAF-Osservatorio Astronomico di Padova, vicolo Osservatorio 5, 35122 Padova, Italy e-mail: [email protected] 2 Dipartimento di Fisica e Astronomia, Università di Padova, vicolo Osservatorio 3, 35122 Padova, Italy 3 SIM, Faculdade de Ciências, Universidade de Lisboa, Ed. C8, Campo Grande, 1749-016 Lisboa, Portugal 4 Institut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, 08028 Barcelona, Spain 5 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, UMR 5804, 33615 Pessac, France Received 26 May 2017 / Accepted 29 January 2018 ABSTRACT Context. The Tycho-Gaia Astrometric Solution (TGAS) subset of the first Gaia catalogue contains an unprecedented sample of proper motions and parallaxes for two million stars brighter than G 12 mag. Aims. We take advantage of the full astrometric solution available∼ for those stars to identify the members of known open clusters and compute mean cluster parameters using either TGAS or the fourth U.S. Naval Observatory CCD Astrograph Catalog (UCAC4) proper motions, and TGAS parallaxes. Methods. We apply an unsupervised membership assignment procedure to select high probability cluster members, we use a Bayesian/Markov Chain Monte Carlo technique to fit stellar isochrones to the observed 2MASS JHKS magnitudes of the member stars and derive cluster parameters (age, metallicity, extinction, distance modulus), and we combine TGAS data with spectroscopic radial velocities to compute full Galactic orbits.
    [Show full text]
  • 108 Afocal Procedure, 105 Age of Globular Clusters, 25, 28–29 O
    Index Index Achromats, 70, 73, 79 Apochromats (APO), 70, Averted vision Adhafera, 44 73, 79 technique, 96, 98, Adobe Photoshop Aquarius, 43, 99 112 (software), 108 Aquila, 10, 36, 45, 65 Afocal procedure, 105 Arches cluster, 23 B1620-26, 37 Age Archinal, Brent, 63, 64, Barkhatova (Bar) of globular clusters, 89, 195 catalogue, 196 25, 28–29 Arcturus, 43 Barlow lens, 78–79, 110 of open clusters, Aricebo radio telescope, Barnard’s Galaxy, 49 15–16 33 Basel (Bas) catalogue, 196 of star complexes, 41 Aries, 45 Bayer classification of stellar associations, Arp 2, 51 system, 93 39, 41–42 Arp catalogue, 197 Be16, 63 of the universe, 28 Arp-Madore (AM)-1, 33 Beehive Cluster, 13, 60, Aldebaran, 43 Arp-Madore (AM)-2, 148 Alessi, 22, 61 48, 65 Bergeron 1, 22 Alessi catalogue, 196 Arp-Madore (AM) Bergeron, J., 22 Algenubi, 44 catalogue, 197 Berkeley 11, 124f, 125 Algieba, 44 Asterisms, 43–45, Berkeley 17, 15 Algol (Demon Star), 65, 94 Berkeley 19, 130 21 Astronomy (magazine), Berkeley 29, 18 Alnilam, 5–6 89 Berkeley 42, 171–173 Alnitak, 5–6 Astronomy Now Berkeley (Be) catalogue, Alpha Centauri, 25 (magazine), 89 196 Alpha Orionis, 93 Astrophotography, 94, Beta Pictoris, 42 Alpha Persei, 40 101, 102–103 Beta Piscium, 44 Altair, 44 Astroplanner (software), Betelgeuse, 93 Alterf, 44 90 Big Bang, 5, 29 Altitude-Azimuth Astro-Snap (software), Big Dipper, 19, 43 (Alt-Az) mount, 107 Binary millisecond 75–76 AstroStack (software), pulsars, 30 Andromeda Galaxy, 36, 108 Binary stars, 8, 52 39, 41, 48, 52, 61 AstroVideo (software), in globular clusters, ANR 1947
    [Show full text]
  • A RAVE Investigation on Galactic Open Clusters II
    A&A 600, A106 (2017) Astronomy DOI: 10.1051/0004-6361/201630012 & c ESO 2017 Astrophysics A RAVE investigation on Galactic open clusters II. Open cluster pairs, groups and complexes? C. Conrad1,??, R.-D. Scholz1, N. V. Kharchenko1; 2; 3, A. E. Piskunov1; 2; 4, S. Röser2, E. Schilbach2, R. S. de Jong1, O. Schnurr1, M. Steinmetz1, E. K. Grebel2, T. Zwitter5, O. Bienaymé6, J. Bland-Hawthorn7, B. K. Gibson8, G. Gilmore9, G. Kordopatis1, A. Kunder1, J. F. Navarro10, Q. Parker11, W. Reid12, G. Seabroke13, A. Siviero14, F. Watson15, and R. Wyse16 1 Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany e-mail: [email protected] 2 Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstraße 12−14, 69120 Heidelberg, Germany 3 Main Astronomical Observatory, 27 Academica Zabolotnogo Str., 03680 Kiev, Ukraine 4 Russian Academy of Science, Institute of Astronomy, 48 Pyatnitskaya, 109017 Moscow, Russia 5 Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000 Ljubljana, Slovenia 6 Observatoire astronomique de Strasbourg, Université de Strasbourg, CNRS, UMR 7550, 11 rue de l’Université, 67000 Strasbourg, France 7 Sydney Institute for Astronomy, School of Physics A28, University of Sydney, NSW 2006, Australia 8 Centre for Astrophysics, Department of Physics and Mathematics, University of Hull, Hull, HU6 7RX, UK 9 Institute of Astronomy, Cambridge University, Madingley Road, Cambridge CB3 0HA, UK 10 Department of Physics and Astronomy, University of Victoria,
    [Show full text]
  • Open Clusters in APOGEE and GALAH Combining Gaia and Ground-Based Spectroscopic Surveys?
    A&A 623, A80 (2019) Astronomy https://doi.org/10.1051/0004-6361/201834546 & c ESO 2019 Astrophysics Open clusters in APOGEE and GALAH Combining Gaia and ground-based spectroscopic surveys? R. Carrera1, A. Bragaglia2, T. Cantat-Gaudin3, A. Vallenari1, L. Balaguer-Núñez3, D. Bossini1, L. Casamiquela4, C. Jordi3, R. Sordo1, and C. Soubiran4 1 INAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, Italy e-mail: [email protected] 2 INAF-Osservatorio di Astrofisica e Scienza dello Spazio, via P. Gobetti 93/3, 40129 Bologna, Italy 3 Institut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, 08028 Barcelona, Spain 4 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France Received 31 October 2018 / Accepted 26 January 2019 ABSTRACT Context. Open clusters are ideal laboratories to investigate a variety of astrophysical topics, from the properties of the Galactic disc to stellar-evolution models. Knowing their metallicity and possibly detailed chemical abundances is therefore important. However, the number of systems with chemical abundances determined from high-resolution spectroscopy remains small. Aims. Our aim is to increase the number of open clusters with radial velocities and chemical abundances determined from high- resolution spectroscopy using publicly available catalogues of surveys in combination with Gaia data. Methods. Open cluster stars have been identified in the APOGEE and GALAH spectroscopic surveys by cross-matching their latest data releases with stars for which high-probability astrometric membership has been derived in many clusters on the basis of the Gaia second data release.
    [Show full text]
  • Arxiv:1801.10042V2 [Astro-Ph.GA] 8 Feb 2018
    Astronomy & Astrophysics manuscript no. article_arXiv ©ESO 2018 February 9, 2018 Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution T. Cantat-Gaudin1, A. Vallenari1, R. Sordo1, F. Pensabene1; 2, A. Krone-Martins3, A. Moitinho3, C. Jordi4, L. Casamiquela4, L. Balaguer-Núnez4, C. Soubiran5, and N. Brouillet5 1 INAF-Osservatorio Astronomico di Padova, vicolo Osservatorio 5, 35122 Padova, Italy 2 Dipartimento di Fisica e Astronomia, Università di Padova, vicolo Osservatorio 3, 35122 Padova, Italy 3 SIM, Faculdade de Ciências, Universidade de Lisboa, Ed. C8, Campo Grande, P-1749-016 Lisboa, Portugal 4 Institut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, E-08028 Barcelona, Spain 5 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, UMR 5804, 33615 Pessac, France Received date / Accepted date ABSTRACT Context. The Tycho-Gaia Astrometric Solution (TGAS) subset of the first Gaia catalogue contains an unprecedented sample of proper motions and parallaxes for two million stars brighter than G ∼ 12 mag. Aims. We take advantage of the full astrometric solution available for those stars to identify the members of known open clusters and compute mean cluster parameters using either TGAS or the fourth U.S. Naval Observatory CCD Astrograph Catalog (UCAC4) proper motions, and TGAS parallaxes. Methods. We apply an unsupervised membership assignment procedure to select high probability cluster members, we use a Bayesian/Markov Chain Monte Carlo technique to fit stellar isochrones to the observed 2MASS JHKS magnitudes of the member stars and derive cluster parameters (age, metallicity, extinction, distance modulus), and we combine TGAS data with spectroscopic radial velocities to compute full Galactic orbits.
    [Show full text]
  • Open Cluster Kinematics with Gaia DR2 ? C
    Astronomy & Astrophysics manuscript no. OC_kinematics_V4 c ESO 2019 March 1, 2019 Open cluster kinematics with Gaia DR2 ? C. Soubiran1, T. Cantat-Gaudin2, M. Romero-Gomez2, L. Casamiquela1, C. Jordi2, A. Vallenari3, T. Antoja2, L. Balaguer-Núñez2, D. Bossini3, A. Bragaglia4, R. Carrera3, A. Castro-Ginard2, F. Figueras2, U. Heiter6, D. Katz7, A. Krone-Martins5, J.-F. Le Campion1, A. Moitinho5, and R. Sordo3 1 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France e-mail: [email protected] 2 Institut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, E-08028 Barcelona, Spain 3 INAF-Osservatorio Astronomico di Padova, vicolo Osservatorio 5, 35122 Padova, Italy 4 INAF-Osservatorio di Astrofisica e Scienza dello Spazio, via Gobetti 93/3, 40129 Bologna, Italy 5 CENTRA, Faculdade de Ciências, Universidade de Lisboa, Ed. C8, Campo Grande, P-1749-016 Lisboa, Portugal 6 Department of Physics and Astronomy, Uppsala University, Box 516, 75120 Uppsala, Sweden 7 GEPI, Observatoire de Paris, Université PSL, CNRS, 5 Place Jules Janssen, 92190 Meudon, France Received March 1, 2019, accepted ABSTRACT Context. Open clusters are very good tracers of the evolution of the Galactic disc. Thanks to Gaia, their kinematics can be investigated with an unprecedented precision and accuracy. Aims. The distribution of open clusters in the 6D phase space is revisited with Gaia DR2. Methods. The weighted mean radial velocity of open clusters was determined, using the most probable members available from a previous astrometric investigation that also provided mean parallaxes and proper motions. Those parameters, all derived from Gaia DR2 only, were combined to provide the 6D phase-space information of 861 clusters.
    [Show full text]
  • Open Clusters in APOGEE and GALAH
    Astronomy & Astrophysics manuscript no. apogee_galah_astroph c ESO 2019 January 29, 2019 Open clusters in APOGEE and GALAH Combining Gaia and ground-based spectroscopic surveys R. Carrera1, A. Bragaglia2, T. Cantat-Gaudin3, A. Vallenari1, L. Balaguer-Núñez3, D. Bossini1, L. Casamiquela4, C. Jordi3, R. Sordo1, and C. Soubiran4 1 INAF-Osservatorio Astronomico di Padova, vicolo dell’Osservatorio 5, 35122 Padova, Italy e-mail: [email protected] 2 INAF-Osservatorio di Astrofisica e Scienza dello Spazio, via P. Gobetti 93/3, 40129 Bologna, Italy 3 Institut de Ciències del Cosmos, Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, E-08028 Barcelona, Spain 4 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, F-33615 Pessac, France Received ; accepted ABSTRACT Context. Open clusters are ideal laboratories to investigate a variety of astrophysical topics, from the properties of the Galactic disk to stellar evolutionary models. Knowing their metallicity and possibly detailed chemical abundances is therefore important. However, the number of systems with chemical abundances determined from high resolution spectroscopy is still small. Aims. To increase the number of open clusters with radial velocities and chemical abundances determined from high resolution spectroscopy we used publicly available catalogues of surveys in combination with Gaia data. Methods. Open cluster stars have been identified in the APOGEE and GALAH spectroscopic surveys by cross-matching their latest data releases with stars for which high-probability astrometric membership has been derived in many clusters on the basis of the Gaia second data release. Results. Radial velocities have been determined for 131 and 14 clusters from APOGEE and GALAH data, respectively.
    [Show full text]
  • A RAVE Investigation on Galactic Open Clusters II
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by HKU Scholars Hub A RAVE investigation on Galactic open clusters II. Open cluster Title pairs, groups and complexes Conrad, C; Scholz, RD; Kharchenko, NV; Piskunov, AE; Röser, S; Schilbach, E; de Jong, RS; Schnurr, O; Steinmetz, M; Grebel, Author(s) EK; Zwitter, T; Bienaymé, O; Bland-Hawthorn, J; Gibson, BK; Gilmore, G; Kordopatis, G; Kunder, A; Navarro, JF; Parker, QA; Reid, W; Seabroke, G; Siviero, A; Watson, F; Wyse, R Citation Astronomy & Astrophysics, 2017, v. 600, p. A106:1-15 Issued Date 2017 URL http://hdl.handle.net/10722/241781 The original publication is available at [journal web site] or Credit: Author, A&A, vol., page, year, reproduced with Rights permission, © ESO; This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. A&A 600, A106 (2017) Astronomy DOI: 10.1051/0004-6361/201630012 & c ESO 2017 Astrophysics A RAVE investigation on Galactic open clusters II. Open cluster pairs, groups and complexes? C. Conrad1,??, R.-D. Scholz1, N. V. Kharchenko1; 2; 3, A. E. Piskunov1; 2; 4, S. Röser2, E. Schilbach2, R. S. de Jong1, O. Schnurr1, M. Steinmetz1, E. K. Grebel2, T. Zwitter5, O. Bienaymé6, J. Bland-Hawthorn7, B. K. Gibson8, G. Gilmore9, G. Kordopatis1, A. Kunder1, J. F. Navarro10, Q. Parker11, W. Reid12, G. Seabroke13, A. Siviero14, F. Watson15, and R. Wyse16 1 Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany e-mail: [email protected] 2 Astronomisches
    [Show full text]
  • 250+ Deep-Sky Objects Visible with 7X35 Binoculars and the Naked-Eye
    6726 1 Scott N. Harrington 2nd edition September, 2018 2 To my family, Who were always understanding of my excursions under the stars. To the late Jack Horkheimer, a.k.a. Star Gazer, Whose television show kept this young astronomer inspired during those crucial first years. I’ll never stop “looking up”. And in memory of my dog Nell, who kept me company many long evenings – especially the one just before she passed away peacefully at the age of fifteen. I owe her a thanks for helping me with my observations by making this young astronomer feel safe at night. You will always be my favorite of our dogs. 3 Acknowledgements Below is a list of books that I read (most for the first time) in the last few years. They were all deeply influential in helping me discover many of the toughest objects that fill out my list. I would like to note that one I have not read, but greatly look forward to doing so, is Richard P. Wilds Bright & Dark Nebulae: An Observers Guide to Understanding the Clouds of the Milky Way Galaxy. Atlas of the Messier Objects by Ronald Stoyan The Backyard Astronomer’s Guide* by Terence Dickinson and Alan Dyer Cosmic Challenge – The Ultimate Observing List for Amateurs by Philip S. Harrington Deep-Sky Companions: The Caldwell Objects by Stephen James O’Meara Deep-Sky Companions: Hidden Treasures by Stephen James O'Meara Deep-Sky Companions: The Messier Objects by Stephen James O’Meara Deep-Sky Companions: The Secret Deep by Stephen James O’Meara Deep-Sky Wonders by Sue French Observing Handbook and Catalogue of Deep-Sky Objects by Christian B.
    [Show full text]