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Related papers: Correlated spectral variability in brown dwarfs

200 papers

We report on the first dedicated monitoring campaign of spectroscopic variability in young brown dwarfs. High-resolution optical spectra of six targets in nearby star-forming regions were obtained over 11 nights between 2005 January-March…

Astrophysics · Physics 2009-11-13 Alexander Scholz , Ray Jayawardhana

In this paper we study the full sample of known Spitzer [$3.6~\mu$m] and $J$-band variable brown dwarfs. We calculate the rotational velocities, $v\sin i$, of 16 variable brown dwarfs using archival Keck NIRSPEC data and compute the…

Solar and Stellar Astrophysics · Physics 2017-06-28 Johanna M. Vos , Katelyn N. Allers , Beth A. Biller

The time scales of variability in active M dwarfs can be related to their various physical parameters. Thus, it is important to understand such variability to decipher the physics of these objects. In this study, we have performed the low…

Solar and Stellar Astrophysics · Physics 2023-08-02 Vipin Kumar , A. S. Rajpurohit , Mudit K. Srivastava , José G. Fernández-Trincado , A. B. A. Queiroz

We present an analysis of brown dwarf model spectra in the mid-infrared spectral region (5 - 20 microns), in anticipation of data obtained with the Space Infrared Telescope Facility. The mid-infrared spectra of brown dwarfs are in several…

Astrophysics · Physics 2007-05-23 D. Saumon , M. S. Marley , K. Lodders

We present two epochs of MPG/ESO 2.2m GROND simultaneous 6-band ($r'i'z'JHK$) photometric monitoring of the closest known L/T transition brown dwarf binary WISE J104915.57-531906.1AB. We report here the first resolved variability monitoring…

In this contribution, I discuss some of the salient features of L and T dwarf spectra in both the red optical (6300--10000 {\AA}) and near-infrared (1--2.5 $\micron$) wavelength regimes. Important absorption bands and lines, including those…

Astrophysics · Physics 2007-05-23 Adam J. Burgasser

We report the discovery of three cool brown dwarfs which fall in the effective temperature gap between the latest L dwarfs currently known, with no methane absorption bands in the 1-2.5um range, and the previously known methane (T) dwarfs,…

Astrophysics · Physics 2010-04-06 S. K. Leggett , T. R. Geballe , Xiaohui Fan

We discuss the behaviour of the JHKL'M' colors of L and T dwarfs, based on photometric and spectroscopic data obtained at the United Kingdom Infrared Telescope in Hawaii. We have measured the first accurate M' photometry for L and T dwarfs.…

Astrophysics · Physics 2007-05-23 S. K. Leggett , D. A. Golimowski , X. Fan , T. R. Geballe , G. R. Knapp

We present photometric light curves for a sample of 21 ultra cool M and L dwarfs in the field and in the young open clusters sigma Orionis and the Pleiades. Evidence for variability with RMS amplitudes (in the I band) of 0.01 to 0.055…

Astrophysics · Physics 2010-11-23 C. A. L. Bailer-Jones , R. Mundt

We present the spectroscopic analysis of a large sample of late-M, L, and T dwarfs from UKIDSS. Using the YJHK photometry from ULAS and the red-optical photometry from SDSS we selected a sample of 262 brown dwarf candidates and we…

Solar and Stellar Astrophysics · Physics 2015-06-24 F. Marocco , H. R. A. Jones , A. C. Day-Jones , D. J. Pinfield , P. W. Lucas , B. Burningham , Z. H. Zhang , R. L. Smart , J. I. Gomes , L. Smith

We present a spectrum of the cool (T_eff = 900 K) brown dwarf Gliese 229B. This spectrum, with a relatively high signal-to-noise ratio per spectral resolution element (> 30), spans the wavelength range from 0.837 microns to 5.0 microns. We…

Astrophysics · Physics 2009-10-30 B. R. Oppenheimer , S. R. Kulkarni , K. Matthews , M. H. van Kerkwijk

We present a 0.6-4.1 micron spectroscopic sequence of M, L, and T dwarfs. The spectra have R~2000 from 0.9 to 2.4 microns and R=2500-200 from 2.9 to 4.1 microns. These new data nearly double the number of L and T dwarfs that have reported…

Astrophysics · Physics 2010-04-06 Michael C. Cushing , John T. Rayner , William D. Vacca

We present an analysis of the 0.95-14.5 micron spectral energy distributions of nine field ultracool dwarfs with spectral types ranging from L1 to T4.5. Effective temperatures, gravities, and condensate cloud sedimentation efficiencies are…

Photometric I band light curves of 21 ultra cool M and L dwarfs are presented. Variability with amplitudes of 0.01 to 0.055 magnitudes (RMS) with typical timescales of an hour to several hours are discovered in half of these objects.…

Astrophysics · Physics 2007-05-23 C. A. L. Bailer-Jones

A large suite of 228 atmospheric retrievals is performed on a curated sample of 19 brown dwarfs spanning the L0 to T8 spectral types using the open-source Helios-r2 retrieval code, which implements the method of short characteristics for…

Earth and Planetary Astrophysics · Physics 2022-05-18 Anna Lueber , Daniel Kitzmann , Brendan P. Bowler , Adam J. Burgasser , Kevin Heng

Brown dwarf spectra offer vital testbeds for our understanding of the chemical and physical processes that sculpt substellar atmospheres. Recently, atmospheric retrieval approaches have been applied to a number of low-resolution (R~100)…

Solar and Stellar Astrophysics · Physics 2023-07-12 Callie E. Hood , Jonathan J. Fortney , Michael R. Line , Jacqueline K. Faherty

[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…

Heterogeneous clouds or temperature perturbations in rotating brown dwarfs produce variability in the observed flux. We report time-resolved simultaneous observations of the variable T6.5 brown dwarf 2MASSJ22282889-431026 over the…

Near-infrared medium-resolution spectra of seven bright brown dwarfs are presented. The spectra were obtained with the Infrared Camera (IRC) on board the infrared astronomical satellite AKARI, covering 2.5--5.0 um with a spectral resolution…

Solar and Stellar Astrophysics · Physics 2015-05-19 Issei Yamamura , Takashi Tsuji , Toshihiko Tanabe

We present multiple-epoch photometric monitoring in the $J$, $H$, and $K_s$ bands of the T1.5 dwarf 2MASS J21392676+0220226 (2M2139), revealing persistent, periodic ($P=7.721\pm$0.005 hr) variability with a peak-to-peak amplitude as high as…

Solar and Stellar Astrophysics · Physics 2015-06-03 Jacqueline Radigan , Ray Jayawardhana , David Lafrenière , Etienne Artigau , Mark Marley , Didier Saumon