Author:
Cappa Cristina E.,Arnal E. Marcelo,Cichowolski Silvina,Goss W. Miller,Pineault Serge
Abstract
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.
Publisher
Cambridge University Press (CUP)
Reference39 articles.
1. Interstellar bubbles. II - Structure and evolution
2. Kinetic efficiencies of stellar wind bubbles
3. St-Louis N. 2002, in: Taylor R. , Landecker T. & Willis A.G. (eds.), Seeing Through the Dust: The Detection of H i and the Exploration of the ISM in Galaxies, ASP-CS 276, 308.
Cited by
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