Observations of the dark cloud in Corona Austrina at 1667 MHz

Observations have been made with the 30 meter dish of the IAR in the direction of the dark cloud in Cr A at the 1667 MHz line of OH. We derived the large-scale distribution of the molecular gas in order to allow an estimation of its mass and a comparison with the dust distribution.

Guardado en:
Detalles Bibliográficos
Autores principales: Cappa, Cristina Elisabet, Pöppel, Wolfgang G. L.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1988
Materias:
Astronomía
Galaxia
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/141981
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
Descripción
Sumario:Observations have been made with the 30 meter dish of the IAR in the direction of the dark cloud in Cr A at the 1667 MHz line of OH. We derived the large-scale distribution of the molecular gas in order to allow an estimation of its mass and a comparison with the dust distribution.

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