New physics of the brown dwarf and L-dwarf atmospheres

Details New physics of the brown dwarf and L-dwarf atmospheres New physics of the brown dwarf and L-dwarf atmospheres

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..415p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 415-420

Physics

Scientific paper

Our main attention is paid for the formation of the spectra of the so-called objects of the Bottom of the Main Sequence. Substellar objects and brown dwarfs lie beyond the lower right end of the Main Sequence. Masses of the very red objects with the low-luminosity are too low for possible nuclear burning of the light elements (hydrogen, lithium or even deuterium) to stop their contraction.

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