1.7k citations · 6.6k across the 38 of their papers we have counts for
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astro-ph.SR2013★ 84 cited
Simulations of protostellar collapse using multigroup radiation hydrodynamics. II. The second collapse
N. Vaytet, G. Chabrier, E. Audit +4
Star formation begins with the gravitational collapse of a dense core inside a molecular cloud. As the collapse progresses, the centre of the core begins to heat up as it becomes o…
astro-ph.SR2013★ 53 cited
Photometric properties of stellar populations in Galactic globular clusters: the role of the Mg-Al anticorrelation
Santi Cassisi, Alessio Mucciarelli, Adriano Pietrinferni +2
We have computed low-mass stellar models and synthetic spectra for an initial chemical composition that includes the full C-N, O-Na, and Mg-Al abundance anticorrelations observed i…