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Radio observations of interstellar bubbles surrounding massive stars

Published online by Cambridge University Press:  26 May 2016

Cristina E. Cappa
Affiliation:
Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa, Buenos Aires, Argentina Facultad de Ciencias Astronómicas y Geofísicas, UNLP, Paseo del Bosque s/n, 1900 La Plata, Argentina
E. Marcelo Arnal
Affiliation:
Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa, Buenos Aires, Argentina Facultad de Ciencias Astronómicas y Geofísicas, UNLP, Paseo del Bosque s/n, 1900 La Plata, Argentina
Silvina Cichowolski
Affiliation:
Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa, Buenos Aires, Argentina
W. Miller Goss
Affiliation:
National Radio Astronomy Observatory, VLA, P.O. Box 0, Socorro, NM 87801, USA
Serge Pineault
Affiliation:
Département de Physique and Observatoire du Mont Mégantic, Université Laval, Ste-Foy, Québec G1K 7P4, Canada

Abstract

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We show radio continuum observations of the WR ring nebulae around WR 101 and WR 113 obtained using the VLA and H i 21 cm line data of the interstellar bubble around the O type stars BD +24° 3866 and BD+25° 3952 obtained with the DRAO Synthesis Telescope. We review previous radio continuum and H i line results toward WR and O-type stars.

Type
Part 4. Feedback from Massive Stars
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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