Discovery of a dense molecular cloud towards a young massive embedded star in 30 Doradus

Context. The 30 Doradus region in the Large Magellanic Cloud is one of the most outstanding star-forming regions of the Local Group and a primary target for studying star formation in an environment of low metallicity. Aims. To obtain a more complete picture of the cool gas that has not yet been con...

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Detalles Bibliográficos
Autores principales: Rubio, M., Paron, S., Dubner, G.
Formato: JOUR
Materias:
HII regions
ISM: individual objects: 30 Doradus
ISM: molecules
Magellanic Clouds
Dense molecular cloud
Emission lines
High sensitivity
Large magellanic clouds
Line emissions
Local groups
Massive stars
Mean density
Metallicities
Molecular clouds
Molecular gas
Molecular hydrogen
Molecular materials
Star formations
Star-forming region
Stellar cluster
Upper limits
Galaxies
Hydrogen
Leakage (fluid)
Molecules
Stars
Clouds
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v505_n1_p177_Rubio
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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