Other
Scientific paper
Aug 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000iraj...27..145p&link_type=abstract
Ir. Astron. J., Vol. 27, No. 2, p. 145 - 149
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2
Brown Dwarfs: Detection, Brown Dwarfs: Masses, Brown Dwarfs: Molecular Clouds
Scientific paper
The population of stellar-like objects, not massive enough to burn hydrogen like normal stars, are known as brown dwarfs. But how low-mass can these mysterious objects be? Also, how many of the lowest-mass brown dwarfs are, as yet, undetected in our Galaxy, or indeed, in other galaxies? To search for more of these elusive objects, the authors have conducted an R- and I-band survey in a region of recent star-formation, the Taurus molecular cloud. Infrared J-, H- and K-band measurements already made for three of the survey candidates indicate that two of these objects are, indeed, young brown dwarfs with masses ≡20 and <10 Jupiter masses.
Fitzsimmons Alan
Fletcher E.
Katsiyannis A.
Mooney C. J.
Pinfield David J.
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