OBSERVED LUMINOSITY SPREAD IN YOUNG CLUSTERS AND FU Ori STARS: A UNIFIED PICTURE
Authors:
- I. BaraffeIBI. Baraffe
- E. VorobyovEVE. Vorobyov
- G. ChabrierGCG. Chabrier
- 21 August 2012
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 756 (2)
Abstract
No abstract availableAll Related Versions
This publication has 59 references indexed in Scilit:
- Spectroscopy of very low mass stars and brown dwarfs in the Lambda Orionis star forming regionAstronomy & Astrophysics, 2011
- Effect of episodic accretion on the structure and the lithium depletion of low-mass stars and planet-hosting starsAstronomy & Astrophysics, 2010
- From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from theHerschelGould Belt SurveyAstronomy & Astrophysics, 2010
- EPISODIC ACCRETION AT EARLY STAGES OF EVOLUTION OF LOW-MASS STARS AND BROWN DWARFS: A SOLUTION FOR THE OBSERVED LUMINOSITY SPREAD IN H-R DIAGRAMS?The Astrophysical Journal, 2009
- Outflows and Jets from Collapsing Magnetized Cloud CoresThe Astrophysical Journal, 2006
- The minimum mass for opacity-limited fragmentation in turbulent cloud coresAstronomy & Astrophysics, 2005
- Dense Cores in Dark Clouds. XIV. N2H+(1–0) Maps of Dense Cloud CoresThe Astrophysical Journal, 2002
- Evolutionary models for low-mass stars and brown dwarfs: Uncertainties and limits at very young agesAstronomy & Astrophysics, 2002
- Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional CalculationsThe Astrophysical Journal, 1998
- Thermonuclear reaction rates VAtomic Data and Nuclear Data Tables, 1988