Author:
André Ph.,Men'shchikov A.,Bontemps S.,Könyves V.,Motte F.,Schneider N.,Didelon P.,Minier V.,Saraceno P.,Ward-Thompson D.,Di Francesco J.,White G.,Molinari S.,Testi L.,Abergel A.,Griffin M.,Henning Th.,Royer P.,Merín B.,Vavrek R.,Attard M.,Arzoumanian D.,Wilson C. D.,Ade P.,Aussel H.,Baluteau J.-P.,Benedettini M.,Bernard J.-Ph.,Blommaert J. A. D. L.,Cambrésy L.,Cox P.,Di Giorgio A.,Hargrave P.,Hennemann M.,Huang M.,Kirk J.,Krause O.,Launhardt R.,Leeks S.,Le Pennec J.,Li J. Z.,Martin P. G.,Maury A.,Olofsson G.,Omont A.,Peretto N.,Pezzuto S.,Prusti T.,Roussel H.,Russeil D.,Sauvage M.,Sibthorpe B.,Sicilia-Aguilar A.,Spinoglio L.,Waelkens C.,Woodcraft A.,Zavagno A.
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference38 articles.
1. The mass function of dense molecular cores and the origin of the IMF
2. André, P., & Saraceno, P. 2005, in The Dusty and Molecular Universe: A Prelude toHerscheland ALMA, ESA SP-577, 179
3. The formation of a star cluster: predicting the properties of stars and brown dwarfs
4. TheHerschelfirst look at protostars in the Aquila rift
5. Chabrier, G. 2005, in The Initial Mass Function 50 years later, ed. E. Corbelli, et al., 41