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相关论文: Proper motion survey and kinematic analysis of the…

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Absolute proper motions are determined for stars and galaxies to V=17.5 over a 450 square-degree area that encloses both Magellanic Clouds. The proper motions are based on photographic and CCD observations of the Yale/San Juan Southern…

We report the results of the first deep, wide-field, near-infrared methane imaging survey of the Rho Ophiuchi cloud core to search for T dwarfs. Among the 6587 objects detected, 22 were identified as T dwarf candidates. Brown dwarf models…

太阳与恒星天体物理 · 物理学 2015-05-19 K. E. Haisch , M. Barsony , C. Tinney

Substellar members of young ($\lesssim$150 Myr) moving groups are valuable benchmarks to empirically define brown dwarf evolution with age and to study the low-mass end of the initial mass function. We have combined Pan-STARRS1 (PS1) proper…

We confirm 66 low-mass stellar and brown dwarf systems (K7-M9) plus 19 visual or spectroscopic companions of the beta Pictoris Moving Group (BPMG). Of these, 41 are new discoveries, increasing the known low-mass members by 45%. We also add…

太阳与恒星天体物理 · 物理学 2017-08-02 Evgenya L. Shkolnik , Katelyn N. Allers , Adam L. Kraus , Michael C. Liu , Laura Flagg

A new proper motion catalog is presented, combining the Sloan Digital Sky Survey (SDSS) with second epoch observations in the r band within a portion of the SDSS imaging footprint. The new observations were obtained with the 90prime camera…

The UKIDSS Large Area Survey (LAS) began in 2005, with the start of the UKIDSS program as a 7 year effort to survey roughly 4000 deg$^2$ at high galactic latitudes in Y, J, H and K bands. The survey also included a significant quantity of…

太阳与恒星天体物理 · 物理学 2013-11-08 L. Smith , P. W. Lucas , B. Burningham , H. R. A. Jones , R. L. Smart , A. H. Andrei , S. Catalan , D. Pinfield

In an effort to identify nearby and unusual cold objects in the solar neighborhood, we searched for previously unidentified moving objects using CatWISE2020 proper motion data combined with machine learning methods. We paired the motion…

Variability is a common characteristic of pre-main-sequence stars (PMS). Near-IR variability surveys of young stellar objects (YSOs) can probe stellar and circumstellar environments and provide information about the dynamics of the on going…

天体物理学 · 物理学 2009-06-23 Catarina Alves de Oliveira , Mark Casali

The kinematic properties of the different classes of objects in a given association hold important clues about its member's history, and offer a unique opportunity to test the predictions of the various models of stellar formation and…

天体物理仪器与方法 · 物理学 2013-06-20 H. Bouy , E. Bertin , E. Moraux , J. -C. Cuillandre , J. Bouvier , D. Barrado , E. Solano , A. Bayo

Context. Galactic globular clusters are a very important tool in explaining the characteristics of the Milky Way. Therefore it is essential to determine the kinematical and dynamical properties of the new star cluster candidates, especially…

Absolute proper motions, their corresponding errors and membership probabilities of 501 stars in the intermediate-age open cluster NGC2548 region are determined from MAMA measurements of 10 photographic plates. The plates have the maximum…

天体物理学 · 物理学 2009-11-07 Z. Y. Wu , K. P. Tian , L. Balaguer-Nunez , C. Jordi , J. L. Zhao , J. Guibert

We associate 132 low-mass ultracool dwarfs in the southern hemisphere as candidate members of five moving groups using photometric and astrometric selection techniques. Of these objects, we present high resolution spectroscopy for seven…

With available Virtual Observatory tools, we looked for new bright blue high proper motion objects in the entire sky: white dwarfs, hot subdwarfs, runaway OB stars, and early-type stars in nearby young moving groups. We performed an all-sky…

太阳与恒星天体物理 · 物理学 2011-05-24 F. M. Jiménez-Esteban , J. A. Caballero , E. Solano

We present an expanded kinematic study of the young cluster NGC 2264 based upon optical radial velocities measured using multi-fiber echelle spectroscopy at the 6.5 meter MMT and Magellan telescopes. We report radial velocities for 695…

太阳与恒星天体物理 · 物理学 2015-06-23 John J. Tobin , Lee Hartmann , Gabor Furesz , Wen-Hsin Hsu , Mario Mateo

A comprehensive census of the stellar content of the nearby OB associations is presented, based on Hipparcos positions, proper motions, and parallaxes. Moving groups are identified by combining de Bruijne's refurbished convergent point…

天体物理学 · 物理学 2009-10-30 P. T. de Zeeuw , R. Hoogerwerf , J. H. J. de Bruijne , A. G. A. Brown , A. Blaauw

We report the discovery of twenty-one hitherto unknown bright southern ultracool dwarfs with spectral types in the range M7 to L5.5, together with new observations of a further three late M dwarfs previously confirmed. Three more objects…

NGC 6809 is a luminous metal-poor halo globular cluster that is relatively easy to study due to its proximity and low concentration. Because of its high Galactic latitude (b = -23deg), interstellar reddening and contamination is not very…

太阳与恒星天体物理 · 物理学 2015-06-05 Devesh P. Sariya , R. K. S. Yadav , A. Bellini

We present a catalogue of near-infrared photometry of young stars associated with the Ophiuchus molecular cloud, based on observations made with the Hubble Space Telescope NICMOS-3 camera at 1.1 $\mu$m and 1.6 $\mu$m. Our survey covers 0.02…

天体物理学 · 物理学 2009-11-07 Lori E. Allen , Philip C. Myers , James Di Francesco , Robert Mathieu , Hua Chen , Erick Young

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