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ALMA-IMF I -- Investigating the Origin of Stellar Masses: Introduction to the Large Program and First Results

F. Motte,S. Bontemps,T. Csengeri,Y. Pouteau,F. Louvet,A. M. Stutz,N. Cunningham,A. Lopez-Sepulcre,N. Brouillet,R. Galvan-Madrid,A. Ginsburg,L. Maud,A. Men'shchikov,F. Nakamura,T. Nony,P. Sanhueza,R. H. Alvarez-Gutierrez,M. Armante,T. Baug,M. Bonfand,G. Busquet,E. Chapillon,D. Diaz-Gonzalez,M. Fernandez-Lopez,A. E. Guzman,F. Herpin,H. -l. Liu,F. Olguin,A. P. M. Towner,J. Bally,C. Battersby,J. Braine,L. Bronfman,H. -R. V. Chen,P. Dell'Ova,J. Di Francesco,M. Gonzalez,A. Gusdorf,P. Hennebelle,N. Izumi,I. Joncour,Y. -n. Lee,B. Lefloch,P. Lesaffre, X. Lu,K. M. Menten, R. Mignon-Risse,J. Molet,E. Moraux,L. Mundy,Q. Nguyen Luong, N. Reyes, Reyes,J. -f. Robitaille,E. Rosolowsky, N. A. Sandoval-Garrido,F. Schuller,B. Svoboda,K. Tatematsu,B. Thomasson, D. Walker, B. Wu,A. P. Whitworth,F. Wyrowski

ASTRONOMY & ASTROPHYSICS（2022）

引用 44|浏览67
关键词
stars: formation,stars: luminosity function, mass function,stars: protostars,ISM: clouds,evolution,H II regions
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