A DRAO and VLA investigation of the environment of WR 130

The environment of the Wolf-Rayet (WR) star WR 130 has been studied using the 21 cm H I line and radio continuum data at 408 and 1420 MHz obtained with the Dominion Radio Astrophysical Observatory (DRAO) Synthesis Telescope. In addition, the H110a recombination line and 21 cm H I line were observed...

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Detalles Bibliográficos
Autores principales: Cichowolski, Silvina, Pineault, Serge, Arnal, Edmundo Marcelo, Testori, Juan Carlos, Goss, W. M., Cappa, Cristina Elisabet
Formato: Articulo
Lenguaje:Inglés
Publicado: 2001
Materias:
Ciencias Astronómicas
astrofísica
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/2054
http://iopscience.iop.org/article/10.1086/323092/meta
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
Descripción
Sumario:The environment of the Wolf-Rayet (WR) star WR 130 has been studied using the 21 cm H I line and radio continuum data at 408 and 1420 MHz obtained with the Dominion Radio Astrophysical Observatory (DRAO) Synthesis Telescope. In addition, the H110a recombination line and 21 cm H I line were observed using the Very Large Array in the DnC and D configurations.

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