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Related papers: A search for southern ultracool dwarfs in young mo…

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We present the full results of our decade-long astrometric monitoring programs targeting 31 ultracool binaries with component spectral types M7-T5. Joint analysis of resolved imaging from Keck Observatory and Hubble Space Telescope and…

Solar and Stellar Astrophysics · Physics 2017-08-09 Trent J. Dupuy , Michael C. Liu

As part of our comprehensive, ongoing characterisation of the low-mass end of the main sequence in the Solar neighbourhood, we used the OSIRIS instrument at the 10.4 m Gran Telescopio Canarias to acquire low- and mid-resolution…

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…

Solar and Stellar Astrophysics · Physics 2015-05-13 Herve Bouy , Eduardo L. Martin

We selected brown dwarf candidates from the seventh Data Release of the Sloan Digital Sky Survey (SDSS DR7) with new photometric selectioncriteria based on a parameteriaztion of well-known L and T dwarfs. Then we confirmed their status with…

Astrophysics of Galaxies · Physics 2010-01-21 Z. H. Zhang , H. R. A. Jones , D. J. Pinfield , R. S. Pokorny , Z. Han

The evolution of brown dwarfs from L to T spectral types is one of the least understood aspects of the ultracool population, partly for lack of a large, well-defined, and well-characterized sample in the L/T transition. To improve the…

We present a spectroscopic and kinematic analysis of 79 nearby M dwarfs in 77 systems. All are low-proper-motion southern hemisphere objects and were identified in a nearby star survey with a demonstrated sensitivity to young stars. Using…

Solar and Stellar Astrophysics · Physics 2017-05-24 Adric R. Riedel , Munazza K. Alam , Emily L. Rice , Kelle L. Cruz , Todd J. Henry

Astrometric observations of resolved binaries provide estimates of orbital periods and will eventually lead to measurement of dynamical masses. Only a few very low mass star and brown dwarf masses have been measured to date, and the…

We aim at developing an efficient method to search for late-type subdwarfs (metal-depleted dwarfs with spectral types >M5) to improve the current statistics. Our objectives are: improve our knowledge of metal-poor low-mass dwarfs, bridge…

Solar and Stellar Astrophysics · Physics 2017-02-08 N. Lodieu , M. Espinoza Contreras , M. R. Zapatero Osorio , E. Solano , M. Aberasturi , E. L. Martin , C. Rodrigo

Aims: Low-resolution optical spectroscopic observations for 78 very low-mass star and brown dwarf candidates that have been photometrically selected using the DENIS survey point source catalogue. Methods: Spectral types are derived for them…

Solar and Stellar Astrophysics · Physics 2015-05-18 E. L. Martin , N. Phan-Bao , M. Bessell , X. Delfosse , T. Forveille , A. Magazzu , C. Reyle , H. Bouy , R. Tata

In this work, we identify 734 ultracool dwarfs with a spectral type of M6 or later, including one L0. Of this sample, 625 were studied spectroscopically for the first time. All of these ultracool dwarfs are within 360~pc, with a…

Solar and Stellar Astrophysics · Physics 2022-04-20 You-Fen Wang , A-Li Luo , Wen-Ping Chen , Hugh R. A. Jones , Bing Du , Yin-Bi Li , Shuo Zhang , Zhong-Rui Bai , Xiao Kong , Yan-Xin Guo

We present a 20-pc, volume-limited sample of M7-L8 dwarfs created through spectroscopic follow-up of sources selected from the Two Micron All Sky Survey (2MASS) Second Incremental Release Point Source Catalog. In this paper, we present…

We present a near-infrared (0.9-2.4 microns) spectroscopic study of 73 field ultracool dwarfs having spectroscopic and/or kinematic evidence of youth (~10-300 Myr). Our sample is composed of 48 low-resolution (R~100) spectra and 41…

Solar and Stellar Astrophysics · Physics 2015-06-16 K. N. Allers , Michael C. Liu

In this research note we identify 130 new M-type candidate members of young associations with the BANYAN $\Sigma$ tool and recently published trigonometric distances from RECONS and URAT-South. We identify a white dwarf candidate in the AB…

Solar and Stellar Astrophysics · Physics 2018-04-17 Jonathan Gagné , Jacqueline K. Faherty , Gilles Fontaine

We present optical spectroscopy and near-infrared photometry of 126 cool white dwarfs in the Sloan Digital Sky Survey (SDSS). Our sample includes high proper motion targets selected using the SDSS and USNO-B astrometry and a dozen…

We present near-infrared (1.15-2.50 microns) medium-resolution (R = 1700) spectroscopy of a sample of 23 brown dwarf candidates in the young Upper Sco association. We confirm membership of 21 brown dwarfs based on their spectral shape,…

Astrophysics · Physics 2009-11-13 N. Lodieu , N. C. Hambly , R. F. Jameson , S. T. Hodgkin

We present an Ultra-Cool Dwarf (UCD) catalogue compiled from low southern Galactic latitudes and mid-plane, from a cross-correlation of the 2MASS and SuperCOSMOS surveys. The catalogue contains 246 members identified from 5042 sq. deg.…

Solar and Stellar Astrophysics · Physics 2015-06-04 S. L. Folkes , D. J. Pinfield , H. R. A. Jones , R. Kurtev , Z. Zhang , M. C. Gálvez-Ortiz , F. Marocco , A. C. Day-Jones , J. R. A. Clarke

We present a study of age-related spectral signatures observed in 25 young low-mass objects that we have previously determined as possible kinematic members of five young moving groups: the Local Association (Pleiades moving group, age=20 -…

A search of the Two Micron All Sky Survey and Sloan Digital Sky Survey reveals 36 previously unknown high proper motion objects with J<17. Their red-optical colors indicate that 27 are M dwarfs, 8 are early-type L dwarfs, and 1 is a…

Astrophysics · Physics 2009-11-13 Scott S. Sheppard , Michael C. Cushing