Triggered massive-star formation at the border of the HII region Sh 104
暂无分享,去创建一个
Astronomy | Granada | University of Wales | Cardiff | A. Whitworth | D. Nadeau | U. Montŕeal | A. Zavagno | L. Deharveng | B. Lefloch | L. D. D. Grenoble | Iram | D. Physics | J. Caplan | S. M. L. D. D. Marseille | Observatoire du Mont Megantic et Departement de Physique
[1] H. Ogawa,et al. The Most Luminous Protostars in Molecular Clouds: A Hint to Understand the Stellar Initial Mass Function , 1999 .
[2] M. M. Moshir,et al. The Midcourse Space Experiment Point Source Catalog, Version 1.2 , 1999 .
[3] B. Elmegreen,et al. Sequential Star Formation in OB Associations: The Role of Molecular Cloud Turbulence , 1995 .
[4] E. Greisen,et al. The NRAO VLA Sky Survey , 1996 .
[5] A. Whitworth,et al. The Preferential Formation of High-Mass Stars in Shocked Interstellar Gas Layers , 1994 .
[6] M. Fich. A VLA Survey of Optically Visible Galactic H II Regions , 1993 .
[7] C. Lada,et al. Sequential formation of subgroups in OB associations , 1977 .
[8] S. Sharpless. A Catalogue of H II Regions. , 1959 .