A very large array 3.6 centimeter continuum survey of galactic wolf-rayet stars

We report the results of a survey of radio continuum emission of Galactic Wolf-Rayet (WR) stars north of δ = -46°. The observations were obtained at 8.46 GHz (3.6 cm) using the Very Large Array, with an angular resolution of ∼6″ × 9″ and typical rms noise of ∼0.04 mJy beam<SUP>-1</SUP>....

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Detalles Bibliográficos
Autores principales:	Cappa, Cristina Elisabet, Goss, W. M., Hucht, K. A. van der
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2004
Materias:	Ciencias Astronómicas Radio continuum: stars Stars: mass loss Stars: Wolf-Rayet
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/83534
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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