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IZ photometry of L dwarfs and the implications for brown dwarf surveys

✍ Scribed by I. A. Steele; L. Howells

Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
121 KB
Volume
313
Category
Article
ISSN
0035-8711

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nous of main sequence stars, having masses 0.1-0.5 times the mass of the Sun. The habitable zones around such stars Planets within the habitable zones of M dwarfs are likely to are therefore very close, being typically between 0.03 and be synchronous rotators; in other words, one side is permanently