From darkness to light : origin and evolution of young stellar clusters : proceedings of a meeting held in Cargèse, Corsica, France, 3-8 April 2000

By T. Montmerle, P. Andre'. 2001

150 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Spectroscopy of Very Low Mass Stars and Brown Dwarfs in IC 2391: Lithium Depletion and Hα Emission (2004, background): “Note, however, that Jeffries & Naylor (2001) have reevaluated the error budget for them, both experimental and systematic, and (R I )C color index (bottom).”
The physics of star formation (2003, background): “…which are often hierachical in structure and contain subgroups (Testi et al 2000; Elmegreen et al 2000); the mass of the most massive star in each subgroup or cluster tends to increase systematically with the mass of the cluster (Larson 1982, 2003; Testi et al 1999, 2001; Garay and Lizano 1999).”
DYNAMICAL MASS SEGREGATION ON A VERY SHORT TIMESCALE (2009, background): “Prestellar cores are often observed to move subsonically (Belloche et al. 2001; André 2002; Walsh et al. 2004; Peretto et al. 2006; Kirk et al. 2007).”