. We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M type) in a two-epoch CCD proper motion survey of 413 square degrees, complemented by infrared photometry from DENIS. One of them has a strong lithium line and is therefore a brown dwarf. The other is a common proper motion companion to the mid-M dwarf LHS 102 (GJ 1001), which has a well determined trigonometric parallax. LHS 102B is thus the coolest L dwarf of known distance and luminosity. Key words: : Galaxy: kinematics and dynamics --- dark matter --- stars: low-mass, brown dwarfs 1. Introduction Two years ago, several very cold dwarfs were identified by DENIS (Delfosse et al., 1997) and Kelu 1 was found through its high proper motion...
International audienceWe report on new nearby L and late-M dwarfs (dphot = 3.0, later than M8.0) at ...
We selected brown dwarf candidates from the seventh Data Release of the Sloan Digital Sky Survey (SD...
We report the discovery of the wide L1.5+L4.5 binary 2MASS J152002244422419AB, identified during spe...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M...
We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M...
Abstract. We report the discovery of three L dwarfs in the solar vicinity within 30 parsecs. These o...
We present a sample of 484 L dwarfs, 210 of which are newly discovered from the Sloan Digital Sky Su...
In recent years brown dwarfs have been extended to a new Y-dwarf class with effective temperatures c...
International audienceWe report on new nearby L and late-M dwarfs (dphot = 3.0, later than M8.0) at ...
Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory ...
International audienceWe report on new nearby L and late-M dwarfs (dphot = 3.0, later than M8.0) at ...
International audienceWe report on new nearby L and late-M dwarfs (dphot = 3.0, later than M8.0) at ...
We selected brown dwarf candidates from the seventh Data Release of the Sloan Digital Sky Survey (SD...
We report the discovery of the wide L1.5+L4.5 binary 2MASS J152002244422419AB, identified during spe...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
5 pages, LaTeX, 6 postscript figures, style correction, two spectra of the discovered objects added,...
We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M...
We report the discovery of two L dwarfs (the new spectral class defined for dwarfs cooler than the M...
Abstract. We report the discovery of three L dwarfs in the solar vicinity within 30 parsecs. These o...
We present a sample of 484 L dwarfs, 210 of which are newly discovered from the Sloan Digital Sky Su...
In recent years brown dwarfs have been extended to a new Y-dwarf class with effective temperatures c...
International audienceWe report on new nearby L and late-M dwarfs (dphot = 3.0, later than M8.0) at ...
Original article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory ...
International audienceWe report on new nearby L and late-M dwarfs (dphot = 3.0, later than M8.0) at ...
International audienceWe report on new nearby L and late-M dwarfs (dphot = 3.0, later than M8.0) at ...
We selected brown dwarf candidates from the seventh Data Release of the Sloan Digital Sky Survey (SD...
We report the discovery of the wide L1.5+L4.5 binary 2MASS J152002244422419AB, identified during spe...