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相关论文: Cool dwarfs stars from the Torino Observatory Para…

200 篇论文

Aims. We try to identify ultra-cool dwarfs from the seventh Data Release of the Sloan Digital Sky Survey (SDSS DR7) with SDSS i-z and r-z colors. We also obtain proper motion data from SDSS, 2MASS, and UKIDSS and improve spectral typing…

Cool subdwarfs are the oldest members of the low mass stellar population. Mostly present in the galactic halo, subdwarfs are characterized by their low metallicity. Measuring their binary fraction and comparing it to solar metallicity stars…

太阳与恒星天体物理 · 物理学 2015-06-23 Carl Ziegler , Nicholas M. Law , Christoph Baranec , Reed L. Riddle , Joshua T. Fuchs

We present Spitzer 5-15 micron spectroscopy of one cool white dwarf and 3.6-8 micron photometry of 51 cool white dwarfs with T_eff < 6000 K. The majority of our targets have accurate BVRIJHK photometry and trigonometric parallax…

太阳与恒星天体物理 · 物理学 2011-02-11 Mukremin Kilic , Piotr M. Kowalski , William T. Reach , Ted von Hippel

We present a detailed spectroscopic and photometric analysis of 219 DA and DB white dwarfs for which trigonometric parallax measurements are available. Our aim is to compare the physical parameters derived from the spectroscopic and…

太阳与恒星天体物理 · 物理学 2017-10-18 Antoine Bédard , Pierre Bergeron , Gilles Fontaine

Based on observations performed with the Pulkovo normal astrograph in 2008-2015 and data from sky surveys (DSS, 2MASS, SDSS DR12, WISE), we have investigated the motions of 1308 stars with proper motions larger than 300 mas/yr down to…

太阳与恒星天体物理 · 物理学 2016-05-02 M. Yu. Khovritchev , A. M. Kulikova

We assembled a catalogue of bright, hot subdwarf and white dwarf stars extracted from a joint ultraviolet, optical, and infrared source list. The selection is secured using colour criteria that correlate well with effective temperatures…

太阳与恒星天体物理 · 物理学 2015-05-19 S. Vennes , A. Kawka , P. Nemeth

We present the results of a search for cool subdwarfs for which our candidates were drawn from a V-J reduced proper-motion diagram constructed by Salim & Gould (2002). Kinematic (U, V, and W) and self-consistent stellar parameters (Teff,…

天体物理学 · 物理学 2009-11-07 David Yong , David L. Lambert

A detailed analysis of halo white dwarf candidates is presented, which is based on model atmosphere fits to observed energy distributions built from photoelectric or photographic magnitudes. Most of the candidates identified in reduced…

天体物理学 · 物理学 2009-11-07 P. Bergeron

We present the Late-Type Extension to the Motion Verified Red Stars (LaTE-MoVeRS) catalog, containing 46,463 photometric late-type ($>$ M5) dwarfs within the Sloan Digital Sky Survey (SDSS) footprint. Proper motions were computed for…

太阳与恒星天体物理 · 物理学 2017-02-08 Christopher A. Theissen , Andrew A. West , Guillaume Shippe , Adam J. Burgasser , Sarah J. Schmidt

We present proper motion measurements for carbon stars found during the APM Survey for Cool Carbon Stars in the Galactic Halo (Totten & Irwin, 1998). Measurements are obtained using a combination of POSSI, POSSII and UKST survey plates…

天体物理学 · 物理学 2010-04-21 E. J. Totten , M. J. Irwin , P. A. Whitelock

Here we present 1584 new southern proper motion systems with mu > 0.18 "/yr and 16.5 > R_59F > 18.0. This search complements the six previous SuperCOSMOS-RECONS (SCR) proper motion searches of the southern sky for stars within the same…

太阳与恒星天体物理 · 物理学 2015-05-28 Mark R. Boyd , Todd J. Henry , Wei-Chun Jao , John P. Subasavage , Nigel C. Hambly

We present a catalog of over 6.2 million stars with measured proper motions. All these stars are observed in the direction of the Magellanic Clouds within the brightness range 12 < I < 19 mag. Based on these proper motions about 440 000…

星系天体物理 · 物理学 2012-04-26 R. Poleski , I. Soszyński , A. Udalski , M. K. Szymański , M. Kubiak , G. Pietrzyński , Ł. Wyrzykowski , K. Ulaczyk

The comparison of optical and 2MASS near-infrared photometry for large samples of catalogued proper motion stars has the potential to discover previously unrecognized nearby objects of rare type. In this paper we present the discovery of…

天体物理学 · 物理学 2009-11-07 Patrick J. Lowrance , J. Davy Kirkpatrick , I. Neill Reid , Kelle L. Cruz , James Liebert

Aims. We demonstrate the feasibility of determining parallaxes for nearby objects with theWide Field Camera on the United Kingdom Infrared Telescope (UKIRT) using the UKIRT Infrared Deep Sky Survey as a first epoch. We determine physical…

Astrometric measurements for 25 red dwarf systems are presented, including the first definitive trigonometric parallaxes for 20 systems within 10 pc of the Sun, the horizon of the RECONS sample. The three nearest systems that had no…

Proper motion measurements of the cool and ultracool populations in the Upper Scorpius OB association are crucial to confirm membership and to identify possible run-away objects. We cross-match samples of photometrically selected and…

太阳与恒星天体物理 · 物理学 2015-05-13 Herve Bouy , Eduardo L. Martin

We present mid-infrared photometry of 124 white dwarf stars with Spitzer Space Telescope. Objects were observed simultaneously at 4.5 and 8.0um with sensitivities better than 1 mJy. This data can be used to test models of white dwarf…

A list of 4,131 dwarfs, subgiants, and giants located, or suspected to be located, within 33 parsecs of the Sun is presented. All the stars are drawn from the new LSPM-north catalog of 61,976 stars with annual proper motions larger than…

天体物理学 · 物理学 2008-11-26 Sebastien Lepine

We report new spectroscopic results, obtained with UKIRT/CGS4, of a sample of 14 candidate ultracool dwarfs selected from the DENIS (Deep Near-Infrared Survey of the Southern Sky) database. A further object, selected from the 2MASS Second…

天体物理学 · 物理学 2009-11-10 T. R. Kendall , X. Delfosse , E. L. Martin , T. Forveille

We describe the 44 systems discovered to be within 10 parsecs of the Sun by the RECONS team, primarily via the long-term astrometry program at CTIO that began in 1999. The systems --- including 41 with red dwarf primaries, 2 white dwarfs,…