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new light on dark stars
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new light on dark stars
Hyperactive brown dwarf has a companion, and may be old and heavy to boot | The Brown Dwarf Blog
https://browndwarf.wordpress.com/2011/07/08/hyperactive-brown-dwarf-has-a-companion-and-may-also-be-old-and-heavy-to-boot
The Brown Dwarf Blog. New light on dark stars. The Burgasser Research Group. First L Dwarf in the Kepler Field. A Very Low Mass Ménage à Trois →. Hyperactive brown dwarf has a companion, and may be old and heavy to boot. Stellar activity is typically attributed to magnetic field interactions, but in brown dwarfs this emission is more of a mystery. For the most part, brown dwarfs. The hyperactive dwarf in question is 2MASS J13153094-2649513. 2MASS 1315-2649 for short), an L-type dwarf. Coming from this so...
A Very Low Mass Ménage à Trois | The Brown Dwarf Blog
https://browndwarf.wordpress.com/2012/08/04/a-very-low-mass-menage-a-trois
The Brown Dwarf Blog. New light on dark stars. The Burgasser Research Group. Hyperactive brown dwarf has a companion, and may be old and heavy to boot. A Very Low Mass Ménage à Trois. The majority of stars like the Sun are found in multiple systems. Nickel Telescope image of SDSS 0006-0852 (at left) and LP 704-48 (at right). The scale of this image is 5 arcminutes on a side, with North up and East toward the left. The M dwarf components of this system – LP 704-48. Using the SpeX spectrograph. On the 3-me...
The Brown Dwarf Blog | new light on dark stars | Page 2
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The Brown Dwarf Blog. New light on dark stars. The Burgasser Research Group. Newer posts →. Clouds on a Young Planet: First Science Results with FIRE. A UKIDSS false color image of the Ross 458 system, composed of a pair of M dwarfs (bright star in upper left corner) and the planetary-mass brown dwarf Ross 458C (circled in lower right corner). Has revealed the presence of rock clouds in the atmosphere of a planetary-mass companion to the nearby Ross 458 system. The source in question is Ross 458C. Only 8...
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The Brown Dwarf Blog | new light on dark stars
The Brown Dwarf Blog. New light on dark stars. The Burgasser Research Group. A Very Low Mass Ménage à Trois. The majority of stars like the Sun are found in multiple systems. Continue reading →. Very low mass stars. SDSS J000649.16-085246.3. Hyperactive brown dwarf has a companion, and may be old and heavy to boot. Stellar activity is typically attributed to magnetic field interactions, but in brown dwarfs this emission is more of a mystery. For the most part, brown dwarfs. Very low mass stars. WISEP J19...
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