The Large Scale IMF-from local studies to large scale Star-formation
Over the past years observations of young and populous star clusters have shown that the stellar IMF appears to be an invariant featureless Salpeter power-law with an exponent α = 2.35 for stars more massive than a few Msolar. A consensus has also emerged that most, if not all, stars form in stellar groups and star clusters, and that the mass
Weidner, Carsten
Fecha de publicación:
5
2009