The embedded cluster IRAS17136 - 3617 associated with the nebulosity GM24

Bibcode
1991MmSAI..62..731T
Tapia, Mauricio
Referencia bibliográfica

Vulcano Workshop on Young Star Clusters and Early Stellar Evolution, Vulcano, Italy, Sept. 16-20, 1991, Proceedings. A92-42951 17-90 Società Astronomica Italiana, Memorie (ISSN 0037-8720), vol. 62, no. 4, 1991, p. 731-736.

Fecha de publicación:
0
1991
Número de autores
1
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
Radio, infrared, and optical observations of the embedded infrared cluster IRAS17136 - 3617 are reviewed. The cluster consists of more than 25 stars with a total stellar mass of 100-400 solar masses embedded deep into a dense molecular cloud of mass 4 x 10,000 solar masses. An extended H II region is found to be expanding outward of the molecular cloud. The peak emission in radio continuum and Br(gamma) line coincides with the brightest infrared source.
Tipo
Sin árbitro
Nubes moleculares
Nebulosas
Cúmulos de estrellas
Formación estelar
Regiones H II

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