Results 31 to 40 of about 45,019 (231)
Brown Dwarfs in the Hyades and Beyond? [PDF]
We have used both the Low-Resolution Imaging Spectrograph and the HIRES echelle spectrograph on the Keck telescopes to obtain spectra of twelve candidate members of the Hyades cluster identified by Leggett and Hawkins (1988, 1989). All of the objects are chromospherically-active, late-type M-dwarfs, with H$ $ equivalent widths varying from 1 to 30 ...
I. Neill Reid, Suzanne L. Hawley
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On the mass segregation of stars and brown dwarfs in Taurus [PDF]
We use the new minimum spanning tree (MST) method to look for mass segregation in the Taurus association. The method computes the ratio of MST lengths of any chosen subset of objects, including the most massive stars and brown dwarfs, to the MST lengths ...
Adams+54 more
core +2 more sources
Intercomparison of Brown Dwarf Model Grids and Atmospheric Retrieval Using Machine Learning
Understanding differences between substellar spectral data and models has proven to be a major challenge, especially for self-consistent model grids that are necessary for a thorough investigation of brown dwarf atmospheres.
Anna Lueber+6 more
doaj +1 more source
Modeling Brown Dwarfs, L Dwarfs, and T Dwarfs [PDF]
In this contribution, I review a subset of our recent efforts in spectral and opacity modeling aimed at guiding the study of brown dwarfs, L dwarfs, and T dwarfs. I discuss theoretical calculations of the alkali line profiles, newly generated CrH opacities, new evidence for refractory rainout in T dwarfs from optical spectral measurements, and the ...
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Searching for weather in brown dwarfs [PDF]
8 pages, 7 figures. To appear in the Monthly Notices of the RAS.
C. G. Tinney, A. J. Tolley
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The “Mysterious” Origin of Brown Dwarfs [PDF]
11 pages, 3 figures, ApJ submitted Error in equation 1 has been corrected.
Aake Nordlund, Paolo Padoan
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Parallaxes of Brown Dwarfs at USNO [PDF]
Trigonometric parallaxes have been measured by Dahn et al. (2002) for 28 cool dwarfs and brown dwarfs, including 17 L dwarfs and three T dwarfs. Broadband CCD and near-IR photometry (VRIz*JHK) have been obtained for these objects and for 24 additional late-type dwarfs. These data have been supplemented with astrometry and photometry from the literature,
Richard L. Walker+12 more
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Interactions between brown-dwarf binaries and Sun-like stars
Several mechanisms have been proposed for the formation of brown dwarfs, but there is as yet no consensus as to which -- if any -- are operative in nature. Any theory of brown dwarf formation must explain the observed statistics of brown dwarfs.
A. Natta+51 more
core +1 more source
After a discussion of the physical processes in brown dwarfs, we present a complete, precise definition of brown dwarfs and of planets inspired by the internal physics of objects between 0.1 and 0.001 M_sun. We discuss observational techniques for characterizing low-luminosity objects as brown dwarfs, including the use of the lithium test and cooling ...
Oppenheimer, Ben R.+2 more
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Searches for brown dwarfs [PDF]
AbstractThis review attempts a brief summary of the numerous and diverse searches for the so-called brown dwarfs, substellar objects having masses between giant planets and the lowest mass M dwarf stars.
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