Mass-Luminosity Relationship and Lithium Depletion for Very Low Mass Stars
Open Access
- 10 March 1996
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 459 (2) , L91
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- CM Draconis and YY Geminorum: Agreement between Theory and ObservationThe Astrophysical Journal, 1995
- Correlations of Coronal X-Ray Emission with Activity, Mass, and Age of the Nearby K and M DwarfsThe Astrophysical Journal, 1995
- New Evolutionary Tracks for Very Low Mass StarsThe Astrophysical Journal, 1995
- Model atmospheres for M (sub)dwarf stars. 1: The base model gridThe Astrophysical Journal, 1995
- The Temperature Scale for Cool Dwarfs1995
- Low-temperature Rosseland opacitiesThe Astrophysical Journal, 1994
- New pre-main-sequence tracks for M less than or equal to 2.5 solar mass as tests of opacities and convection modelThe Astrophysical Journal Supplement Series, 1994
- The mass-luminosity relation for stars of mass 1.0 to 0.08 solar massThe Astronomical Journal, 1993
- An expanded set of brown dwarf and very low mass star modelsThe Astrophysical Journal, 1993
- Theoretical models of low-mass stars and brown dwarfs. I - The lower main sequenceThe Astrophysical Journal, 1989