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Increased brain size of the dwarf Channel Island fox (Urocyon littoralis) challenges "Island Syndrome" and suggests little evidence of domestication. [PDF]
PLoS OneSchoenberger KA, Wang X, Edmands S.
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Formation of free-floating planetary mass objects via circumstellar disk encounters. [PDF]
Sci AdvFu Z, Deng H, Lin DNC, Mayer L.
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Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 MJ
De Furio M +13 more
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Science, 2000
ASTRONOMY Dwarfs are low mass, very cool, main-sequence stars, and recent large-scale star surveys have identified a new spectral class, called the L-dwarfs. The low estimated masses of L-dwarfs suggest that most of these objects are brown dwarfs that are rich in hydrides rather than methane. McLean et al. have obtained high-resolution spectra of six L-
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ASTRONOMY Dwarfs are low mass, very cool, main-sequence stars, and recent large-scale star surveys have identified a new spectral class, called the L-dwarfs. The low estimated masses of L-dwarfs suggest that most of these objects are brown dwarfs that are rich in hydrides rather than methane. McLean et al. have obtained high-resolution spectra of six L-
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The Classification of L Dwarfs
2001To highlight the need for new spectral types, a brief review of the discovery of very low luminosity dwarfs — cooler than type M9.5 — is presented. The reasoning behind the choice of letters “L” and “T” is also given. Our philosophy of spectral classification is explained and we use this philosophy to construct an L dwarf typing scheme.
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