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Related papers: Four nearby L dwarfs

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We present the results of a series of short radio observations of six ultracool dwarfs made using the upgraded VLA in S (2--4GHz) and C (4--7GHz) bands. LSR J1835+3259 exhibits a 100 percent right-hand circularly polarised burst which shows…

Solar and Stellar Astrophysics · Physics 2016-12-21 Y. T. Metodieva , A. A. Kuznetsov , A. E. Antonova , J. G. Doyle , G. Ramsay , K. Wu

We report discovery of a young 0.32" L dwarf binary, SDSS J2249+0044AB, found as the result of a Keck LGSAO imaging survey of young field brown dwarfs. Weak K, Na, and FeH features as well as strong VO absorption in the integrated-light…

Solar and Stellar Astrophysics · Physics 2014-11-20 K. N. Allers , Michael C. Liu , Trent J. Dupuy , Michael C. Cushing

We have observed the eclipsing, post-common envelope white dwarf-brown dwarf binary, SDSS141126.20+200911.1, in the near-IR with the HAWK-I imager, and present here the first direct detection of the dark side of an irradiated brown dwarf in…

Solar and Stellar Astrophysics · Physics 2018-10-10 S. L. Casewell , S. P. Littlefair , S. G. Parsons , T. R. Marsh , J. J. Fortney , M. S. Marley

We present two confirmed wide separation L-dwarf common proper motion companions to nearby stars and one candidate identified from the Two Micron All Sky Survey. Spectral types from optical spectroscopy are L0 V, L2.5 V, and L8 V.…

We report preliminary results of a deep near-infrared search for methane-absorbing brown dwarfs; almost five years after the discovery of Gl 229b, there are only a few confirmed examples of this type of object. New J band, wide-field…

Astrophysics · Physics 2009-10-31 T. M. Herbst , D. Thompson , R. Fockenbrock , H. -W. Rix , S. V. W. Beckwith

Aims: We aim to study the near-infrared variability of the T8 dwarfs 2MASS J09393548-2448279 and EQ J1959-3338 by analyzing their $J$-band photometric signal, which can provide new insights into the atmospheric dynamics of cold brown…

Solar and Stellar Astrophysics · Physics 2025-04-30 P. A. Miles-Páez , S. Metchev , M. R. Zapatero Osorio , D. Martín-Carrero

The luminous infrared-loud quasar IRAS 13349+2438 was observed with the XMM-Newton Observatory as part of the Performance Verification program. The spectrum obtained by the Reflection Grating Spectrometer (RGS) exhibits broad (v ~ 1400 km/s…

Trigonometric parallax determinations are presented for 28 late type dwarfs and brown dwarfs, including eight M dwarfs with spectral types between M7 and M9.5, 17 L dwarfs with spectral types between L0 and L8, and three T dwarfs. Broadband…

Surveys have shown that up to one tenth of all ultracool dwarfs (UCDs) are appreciable radio emitters, with their emission attributed to a combination of gyrosynchrotron radiation and the electron cyclotron maser instability (ECMI). 2M…

Solar and Stellar Astrophysics · Physics 2020-07-03 Qicheng Zhang , Gregg Hallinan , Walter Brisken , Stephen Bourke , Aaron Golden

We present new infrared spectra of the T8 brown dwarf 2MASS J04151954-0935066: 2.9-4.1 micron spectra obtained with the Infrared Camera and Spectrograph on the Subaru Telescope, and 5.2-14.5 micron spectra obtained with the Infrared…

[abbreviated] We report resolved near-infrared spectroscopic monitoring of the nearby L dwarf/T dwarf binary WISE J104915.57-531906.1AB (Luhman 16AB), as part of a broader campaign to characterize the spectral energy distribution and…

We present ultra-high resolution (0.32 km/s) spectra obtained with the 3.9m Anglo-Australian Telescope (AAT) and Ultra-High-Resolution Facility (UHRF), of interstellar NaI D1, D2, Ca II K, K I and CH absorption toward two high galactic…

Astrophysics · Physics 2009-10-30 M. S. Sahu , J. C. Blades , L. He , D. Hartmann , M. J. Barlow , I. A. Crawford

We discover four high proper motion L dwarfs by comparing the Wide-field Infrared Survey Explorer (WISE) to the Two Micron All Sky Survey (2MASS). WISE J140533.32+835030.5 is an L dwarf at the L/T transition with a proper motion of…

We present an L-band spectrum of the Ultraluminous Infrared Galaxy IRAS 19254-7245 (the Superantennae), obtained with VLT-ISAAC. The high signal to noise ratio allows a study of the main spectral features with unprecedented detail for an…

We discuss methods for classifying T dwarfs based on spectral morphological features and indices. T dwarfs are brown dwarfs which exhibit methane absorption bands at 1.6 and 2.2 ${\mu}m$. Spectra at red optical (6300--10100 {\AA}) and…

Astrophysics · Physics 2007-05-23 Adam J. Burgasser , J. Davy Kirkpatrick , Michael E. Brown

We present Gemini near-infrared spectroscopic observations of six luminous quasars at z=5.8$\sim$6.3. Five of them were observed using Gemini-South/GNIRS, which provides a simultaneous wavelength coverage of 0.9--2.5 $\mu$m in cross…

We report the discovery of an L-type companion to the young M3.5V star 2MASS J01225093-2439505 at a projected separation of 1.45" (~52 AU) as part of our adaptive optics imaging search for extrasolar giant planets around young low-mass…

Solar and Stellar Astrophysics · Physics 2015-06-16 Brendan P. Bowler , Michael C. Liu , Evgenya L. Shkolnik , Trent J. Dupuy

We confirm the substellar nature of ULAS J141623.94+134836.3, a common proper motion companion to the blue L dwarf SDSS J141624.08+134826.7 identified by Burningham et al. and Scholz. Low-resolution 0.8-2.4 micron spectroscopy obtained with…

Solar and Stellar Astrophysics · Physics 2015-05-18 Adam J. Burgasser , Dagny L. Looper , John T. Rayner

We present near-infrared spectra of seven radio-loud quasars with a median redshift of 2.1, five of which were previously known to have Ly alpha nebulae. Extended [OIII]5007 and H alpha emission are evident around six objects, at the level…

Astrophysics · Physics 2009-10-31 R. J. Wilman , R. M. Johnstone , C. S. Crawford

We present the results of photometric and spectroscopic follow-ups of the lowest mass member candidates in the nearest OB association, Upper Scorpius (5-10 Myr; 145+/-17 pc), with the Gran Telescopio de Canarias (GTC) and European Southern…

Solar and Stellar Astrophysics · Physics 2017-11-15 N. Lodieu , M. R. Zapatero Osorio , V. J. S. Bejar , K. Pena Ramirez