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Related papers: A focus on L dwarfs with trigonometric parallaxes

200 papers

We are currently undertaking a program aimed at identifying previously-unrecognised late-type dwarfs within 20 parsecs of the Sun. As a first step, we have cross-referenced Luyten's NLTT proper motion catalogue against the second…

Astrophysics · Physics 2009-11-07 I. Neill Reid , Kelle L. Cruz

We present a detailed analysis of the white dwarf luminosity functions derived from the local 40 pc sample and the deep proper motion catalog of Munn et al (2014, 2017). Many of the previous studies ignored the contribution of thick disk…

We have identified eight to ten new cool white dwarfs from the Large Area Survey (LAS) Data Release 9 of the United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS). The data set was paired with the Sloan Digital Sky…

Solar and Stellar Astrophysics · Physics 2014-05-02 P. -E. Tremblay , S. K. Leggett , N. Lodieu , B. Freytag , P. Bergeron , J. S. Kalirai , H. -G. Ludwig

This paper presents new trigonometric parallaxes and proper motions for 214 stars. The measurements were made at the US Naval Observatory Flagstaff Station (NOFS) between 1989 and 2017, and the average uncertainty in the parallax values is…

We report on the results of an I-band photometric variability survey of eighteen L dwarfs. We find that seven exhibit statistically significant variations above the 95.4% confidence level with root-mean-square scatter (including photometric…

We present a statistical parallax analysis of low-mass dwarfs from the Sloan Digital Sky Survey (SDSS). We calculate absolute r-band magnitudes (M_r) as a function of color and spectral type, and investigate changes in M_r with location in…

Solar and Stellar Astrophysics · Physics 2015-05-27 John J. Bochanski , Suzanne L. Hawley , Andrew A. West

We present new L' (3.75 um) photometry of six L and T dwarfs, and M' (4.70 um) photometry of ten L and T dwarfs, observed at Gemini Observatory, and new 3.55, 4.49, 5.73 and 7.87 um photometry of nine L and T dwarfs, obtained with the…

Astrophysics · Physics 2008-11-26 S. K. Leggett , D. Saumon , M. S. Marley , T. R. Geballe , D. A. Golimowski , D. Stephens , X. Fan

We report the results of an infrared Doppler survey designed to detect brown dwarf and giant planetary companions to a magnitude-limited sample of ultracool dwarfs. Using the NIRSPEC spectrograph on the Keck II telescope, we obtained…

Solar and Stellar Astrophysics · Physics 2015-05-19 Cullen H. Blake , David Charbonneau , Russel J. White

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

Over the past decade, the BeSSeL Survey and the VERA project have measured trigonometric parallaxes to approximately 250 massive, young stars using VLBI techniques. These sources trace spiral arms over nearly half of the Milky Way. What is…

Instrumentation and Methods for Astrophysics · Physics 2022-09-21 Mark J Reid

Juvenile ultracool dwarfs are late spectral type objects (later than ~M6) with ages between 10 Myr and several 100 Myr. Their age-related properties lie intermediate between very low mass objects in nearby star-forming regions (ages 1-5…

The census of the solar neighborhood is almost complete for stars and becoming more complete in the brown dwarf regime. Spectroscopic, photometric and kinematic characterization of nearby objects helps us to understand the local mass…

Solar and Stellar Astrophysics · Physics 2015-11-04 J. C. Beamín , V. D. Ivanov , D. Minniti , R. L. Smart , K. Muzic , R. A. Mendez , Y. Beletsky , A. Bayo , M. Gromadzki , R. Kurtev

We report, for the first time, photometric variability of L dwarfs in $R$ band. Out of three L1 dwarfs (2MASS 1300+19, 2MASS 1439+19, and 2MASS 1658+70) observed, we have detected R band variability in 2MASS 1300+19 and 2MASS 1439+19. The…

Astrophysics · Physics 2009-11-10 M. Maiti , S. Sengupta , P. S. Parihar , G. C. Anupama

We present a magnitude and proper motion limited catalogue of ~10,000 white dwarf candidates, obtained from the SuperCOSMOS Sky Survey by means of reduced proper motion selection. This catalogue extends to magnitudes r~19.75 and proper…

Astrophysics of Galaxies · Physics 2011-04-21 Nicholas Rowell , Nigel Hambly

We present parallax observations and a detailed model atmosphere analysis of 54 cool and ultracool ($T_{\rm eff}$ < 4000 K) white dwarfs (WDs) in the solar neighbourhood. For the first time, a large number of cool and ultracool WDs have…

Solar and Stellar Astrophysics · Physics 2015-06-24 A. Gianninas , B. Curd , John R. Thorstensen , Mukremin Kilic , P. Bergeron , Jeff J. Andrews , Paul Canton , M. A. Agüeros

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…

Astrophysics · Physics 2009-11-10 J. R. Thorstensen , J. D. Kirkpatrick

We present precise measurements of radial (RV) and projected rotational ($v\sin{i}$) velocities, effective temperatures, and surface gravities of a sample of 258 M6 to L2 dwarfs with multi-epoch, high-resolution ($\lambda/\Delta\lambda$ =…

The variability and rotation of ultra cool dwarfs (UCDs) provide important information on their atmospheres and evolution. As part of an ongoing program to investigate this, projected rotation speeds, vsini, are presented for 16 field UCDs…

Astrophysics · Physics 2009-11-10 C. A. L. Bailer-Jones

We present here the results of astrometric, photometric and spectroscopic observations leading to the determination of the orbit and dynamical masses of the binary L dwarf 2MASSW J0746425+2000321. High angular resolution observations spread…