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相关论文: Discovery of a New Nearby Star

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We present the discovery of a previously unknown very nearby star - LHS 2090 at a distance of only d=6 pc. In order to find nearby (i.e. d < 25 pc) red dwarfs, we re-identified high proper motion stars ($\mu >$ 0.18 arcsec/yr) from the NLTT…

天体物理学 · 物理学 2016-08-30 R. -D. Scholz , H. Meusinger , H. Jahreiß

We report the discovery of seven high proper motion stars with proper motions between about 0.7 and 2.2 arcsec/yr. They were detected in an archival search using multi-epoch positions in the optical SuperCOSMOS Sky Surveys and in the…

天体物理学 · 物理学 2009-11-10 R. -D. Scholz , I. Lehmann , I. Matute , H. Zinnecker

Five new objects with proper motions between 1.0 arcsec/yr and 2.6 arcsec/yr have been discovered via a new RECONS search for high proper motion stars utilizing the SuperCOSMOS Sky Survey. The first portion of the search, discussed here, is…

天体物理学 · 物理学 2009-11-10 N. C. Hambly , T. J. Henry , J. Subasavage , M. Brown , W. -C. Jao

We report the discovery of 182 new southern stars with proper motion larger than 0.45''/yr. The stars were found in an expansion of the SUPERBLINK proper motion survey to 8,980 square degrees south of Decl.=-30. The new high proper motion…

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

We report the discovery of 141 new high proper motion systems (1.0"/yr > mu >= 0.4"/yr) in the southern sky (Declination = -90 degrees to -47 degrees) brighter than UKST plate R_{59F} = 16.5 via our SuperCOSMOS-RECONS (SCR) search. When…

天体物理学 · 物理学 2009-11-10 John P. Subasavage , Todd J. Henry , Nigel C. Hambly , Misty A. Brown , Wei-Chun Jao

High proper motion stars probe several extreme stellar populations, including nearby objects, Galactic halo stars, and hyper-velocity stars. Extending the search for high proper motion stars, to faint limits can increase their numbers and…

太阳与恒星天体物理 · 物理学 2018-12-26 Noam Segev , Eran O. Ofek

We have conducted a systematic search for high proper motion stars in the Digitized Sky Survey, in the area of the sky north of -2.8 degrees in declination and within 25 degrees of the galactic plane. Using the SUPERBLINK software, a…

天体物理学 · 物理学 2011-03-28 Sebastien Lepine , Michael M. Shara , R. Michael Rich

Precise proper motion measurements (sigma_mu ~ 10 mkas/yr) of the recently discovered hyper-velocity star (HVS) SDSS J090745.0+024507 would yield significant constraints on the axis ratios and orientation of a triaxial model for the…

天体物理学 · 物理学 2009-11-13 Oleg Y. Gnedin , Andrew Gould , Jordi Miralda-Escude , Andrew R. Zentner

We present the results of a search for High Proper Motion (HPM) stars, i.e. the ones with \mu > 100 mas/yr, in the direction to the Magellanic Clouds. This sky area was not examined in detail as the high stellar density hampers efforts in…

太阳与恒星天体物理 · 物理学 2011-10-12 R. Poleski , I. Soszynski , A. Udalski , M. K. Szymanski , M. Kubiak , G. Pietrzynski , L. Wyrzykowski , K. Ulaczyk

We present the first results from the Southern Infrared Proper Motion Survey. Using 2 Micron All Sky Survey data along with that of the SuperCOSMOS sky survey we have been able to produce the first widefield infrared proper motion survey.…

天体物理学 · 物理学 2009-11-10 N. R. Deacon , N. C. Hambly , J. A. Cooke

Hypervelocity stars (HVSs) travel with velocities so extreme that dynamical ejection from a massive black hole is their only suggested origin. Following our discovery of the first HVS, we have undertaken a dedicated survey for more HVSs in…

天体物理学 · 物理学 2009-11-11 Warren R. Brown , Margaret J. Geller , Scott J. Kenyon , Michael J. Kurtz

We report the discovery of a nearby M dwarf star, found accidentally while observing the old nova DN Gem at the Wise Observatory. The star is designated 1200-05296925 in the PMM USNO-A1.0 catalogue and its coordinates, calculated for 1997…

天体物理学 · 物理学 2007-05-23 Ohad Shemmer , Shai Kaspi

We present astrometric parallaxes for 18 suspected nearby stars selected from the LSPM-north proper motion catalog. Sixteen objects are confirmed to be main sequence M dwarfs within 16 parsecs of the Sun, including three stars (LSPM…

太阳与恒星天体物理 · 物理学 2009-11-13 Sebastien Lepine , John R. Thorstensen , Michael M. Shara , R. Michael Rich

We present measurements of positions and relative proper motions in the 30 Doradus region of the Large Magellanic Cloud (LMC). We detail the construction of a single-epoch astrometric reference frame, based on specially-designed…

太阳与恒星天体物理 · 物理学 2015-09-16 I. Platais , R. P. van der Marel , D. J. Lennon , J. Anderson , A. Bellini , E. Sabbi , H. Sana , L. R. Bedin

Completion of the SUPERBLINK proper motion survey in the southern celestial hemisphere has turned up 170 new stars with proper motion 0.45 arcsec/yr < pm < 2.0 arcsec/yr. This fourth and final installment completes the all-sky, data-mining…

天体物理学 · 物理学 2009-11-13 Sebastien Lepine

A field star serendipitously observed in a parallax program proved to have a proper motion of 562 mas/yr and a parallax of 82 +- 2 mas. The star is identified with 2MASS J07003664+3157266. A Keck LRIS spectrum shows its spectral type to be…

天体物理学 · 物理学 2009-11-10 J. R. Thorstensen , J. D. Kirkpatrick

We define an enhanced spectral classification scheme for M dwarf stars, and use it to derive spectral classification of 104 northern stars with proper motions larger than 0.5"/yr which we discovered in a survey of high proper motion stars…

天体物理学 · 物理学 2009-11-07 Sebastien Lepine , R. Michael Rich , Michael M. Shara

We have conducted a novel search of most of the southern sky for nearby red dwarfs having low proper motions, with specific emphasis on those with proper motion < 0.18 arcsec yr-1, the lower cutoff of Luyten's classic proper motion catalog.…

We present spectra of 59 nearby stars candidates, M dwarfs and white dwarfs, previously identified using high proper motion catalogues and the DENIS database. We review the existing spectral classification schemes and spectroscopic parallax…

天体物理学 · 物理学 2009-11-11 C. Reyle , R. -D. Scholz , M. Schultheis , A. C. Robin , M. Irwin

Hyper-velocity stars (HVS) are moving so fast that they are unbound to the Galaxy. Dynamical ejection by a supermassive black hole is favoured to explain their origin. Locating the place of birth of an individual HVS is of utmost importance…

太阳与恒星天体物理 · 物理学 2015-05-14 A. Tillich , N. Przybilla , R. -D. Scholz , U. Heber
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