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Related papers: The ages of L dwarfs

200 papers

We have exploited the very precise parallaxes, proper motions and photometry of \textit{Gaia}\, Data Release~2 to study white dwarf members of the Hyades star cluster. Gaia photometry and parallaxes for the eight DA white dwarfs confirmed…

Solar and Stellar Astrophysics · Physics 2018-09-26 M. Salaris , L. R. Bedin , .

We have derived a new age estimate for the nearby young star AB Dor and have investigated the resulting implications for testing theoretical evolutionary models with the data reported by Close and coworkers for the low-mass companion AB Dor…

Astrophysics · Physics 2009-11-13 K. L. Luhman , John R. Stauffer , E. E. Mamajek

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…

Young brown dwarfs share many properties with directly imaged giant extrasolar planets. They therefore provide unique laboratories for investigating the full range of temperature and mass encompasses by the growing collection of planets…

Solar and Stellar Astrophysics · Physics 2017-04-12 Adam C. Schneider , James Windsor , Michael C. Cushing , J. Davy Kirkpatrick

While following up L dwarf candidates selected photometrically from the Two Micron All Sky Survey, we uncovered an unusual object designated 2MASS J01415823-4633574. Its optical spectrum exhibits very strong bands of vanadium oxide but…

We apply a self-consistent and robust Bayesian statistical approach to determining the ages, distances, and ZAMS masses of 28 field DA white dwarfs with ages of approximately 4 to 8 Gyrs. Our technique requires only quality optical and…

Solar and Stellar Astrophysics · Physics 2016-02-19 Erin M. O'Malley , Ted von Hippel , David van Dyk

We combine optical, near-infrared and mid-infrared spectra and photometry to construct expanded spectral energy distributions (SEDs) for 145 field age (\textgreater 500 Myr) and 53 young (lower age estimate \textless 500 Myr) ultracool…

Solar and Stellar Astrophysics · Physics 2015-09-23 Joseph C. Filippazzo , Emily L. Rice , Jacqueline Faherty , Kelle L. Cruz , Mollie M. Van Gordon , Dagny L. Looper

We searched for binary companions to 20 young brown dwarfs in the Upper Scorpius association (145 pc, 5 Myr, nearest OB association) with the the Laser Guide Star adaptive optics system and the facility infrared camera NIRC2 on the 10 m…

Solar and Stellar Astrophysics · Physics 2015-05-27 Beth Biller , Katelyn Allers , Michael Liu , Laird Close , Trent Dupuy

We report the discovery of an L dwarf companion to the A3V star \beta{} Circini. VVV J151721.49-585131.5, or \beta{} Cir B, was identified in a proper motion and parallax catalogue of the Vista Variables in the V\'{i}a L\'{a}ctea survey as…

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…

Astrophysics · Physics 2009-11-10 T. R. Kendall , X. Delfosse , E. L. Martin , T. Forveille

Ultra-cool dwarfs have been defined as dwarfs with spectral types of M7 or later (Kirkpatrick, Henry, & Irwin 1997) and thus include the new L and T spectral classes. The previous IAU report on ultra-cool dwarfs in 1999 described the…

Astrophysics · Physics 2007-05-23 K. L. Luhman

By using images taken with WFCAM on UKIRT and SofI on the NTT and combining them with 2MASS we have measured proper motions for 126 L and T dwarfs in the dwarf archive. Two of these L dwarfs appear to have M dwarf common proper motion…

Astrophysics · Physics 2009-11-13 S. L. Casewell , R. F. Jameson , M. R. Burleigh

We aim to provide a detailed characterization of near-infrared spectra for young LT brown dwarfs, including robust spectral typing, calibrating spectral indices, identifying possible binaries, and selecting suitable spectral standards. We…

Solar and Stellar Astrophysics · Physics 2024-05-29 L. Piscarreta , K. Mužić , V. Almendros-Abad , A. Scholz

We have completed a high-resolution (R=60,000) optical spectroscopic survey of 185 nearby M dwarfs identified using ROSAT data to select active, young objects with fractional X-ray luminosities comparable to or greater than Pleiades…

Solar and Stellar Astrophysics · Physics 2014-11-18 Evgenya Shkolnik , Michael C. Liu , I. Neill Reid

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 report new parallax measurements for ten L and early T type dwarfs, five of which have no previous published values, using observations over 3 years at the robotic Liverpool Telescope. The resulting parallaxes and proper motions have…

Solar and Stellar Astrophysics · Physics 2018-05-23 Y. Wang , R. L. Smart , Z. Shao , H. R. A Jones , F. Marocco , A. Luo , A. Burgasser , J. Zhong , B. Du

We present preliminary results from a coronagraphic survey of young nearby Sun-like stars using the Palomar and Keck adaptive optics systems. We have targeted 251 solar analogs (F5-K5) at 20-160 pc from the Sun, spanning the 3-3000 Myr age…

Astrophysics · Physics 2015-06-10 Stanimir Metchev , Lynne Hillenbrand

We present the results of a long term orbit monitoring program, using sparse aperture masking observations taken with NIRC2 on the Keck-II telescope, of seven G to M-type members of the Upper Scorpius subgroup of the Sco-Cen OB association.…

Solar and Stellar Astrophysics · Physics 2016-02-17 Aaron C. Rizzuto , Michael J. Ireland , Trent J Dupuy , Adam L. Kraus

We report the discovery of a wide (approximately 400 AU projected separation), common proper motion companion to the nearby M dwarf LHS 2803 (PSO J207.0300-13.7422). This object was discovered during our census of the local T dwarf…

(Abridged) The nature of S Ori 70, a faint mid-T type object found towards the direction of the young sigma Orionis cluster, is still under debate. We intend to disentangle whether it is a field brown dwarf or a 3-Myr old planetary-mass…