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Molecular and atomic hydrogen in the environment of hot, massive stars

Published online by Cambridge University Press:  25 May 2016

Nicole St-Louis ,
S. Gervais ,
Thierry Morel  and
Rene Doyon
Nicole St-Louis
Affiliation:
Département de Physique, Université de Montréal, C.P. 6128, Succ. Centre Ville, Montréal (Qc), ESC 3J7, Canada
S. Gervais
Affiliation:
Département de Physique, Université de Montréal, C.P. 6128, Succ. Centre Ville, Montréal (Qc), ESC 3J7, Canada
Thierry Morel
Affiliation:
Imperial College of Science, Technology and Medicine, Blackett Laboratory, Prince Consort Road, London SW7 2BZ, UK
Rene Doyon
Affiliation:
Département de Physique, Université de Montréal, C.P. 6128, Succ. Centre Ville, Montréal (Qc), ESC 3J7, Canada

Extract

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Studies of the atomic and molecular components of the interstellar medium in the vicinity of hot, massive stars have the potential of revealing a wealth of information on the way the star affects the distribution and physical state of the surrounding ISM during its various evolutionary phases, as well as potentially providing some information on the star itself and its past evolution.

Type
Part 3. Interaction of Wolf-Rayet stars and other hot massive stars with their environment: colliding winds and ring nebulae
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 392 - 393
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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St-Louis, N., Gervais, S. 1999, AJ submitted Google Scholar