Hostname: page-component-7bb8b95d7b-pwrkn Total loading time: 0 Render date: 2024-09-24T16:38:32.723Z Has data issue: false hasContentIssue false

The interstellar medium local to HD 10125 (O9.7II)

Published online by Cambridge University Press:  26 May 2016

Silvina Cichowolski
Affiliation:
Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa, Buenos Aires, Argentina
E. Marcelo Arnal
Affiliation:
Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa, Buenos Aires, Argentina Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional La Plata, 1900 La Plata, Argentina
Cristina E. Cappa
Affiliation:
Instituto Argentino de Radioastronomía, C.C. 5, 1894 Villa Elisa, Buenos Aires, Argentina Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional La Plata, 1900 La Plata, Argentina
Sergey Pineault
Affiliation:
Département de Physique, Université Laval, Ste-Foy, Québec G1K 7P4, Canada Observatoire du Mont Mégantic, Notre-Dame-des-Bois, Canada
Nicole St-Louis
Affiliation:
Observatoire du Mont Mégantic, Notre-Dame-des-Bois, Canada Département de Physique, Université de Montréal, CP 6128, Succursale Centre Ville, Montréal, Québec H3C 3J7, Canada

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The structure and dynamics of the interstellar medium (ISM) are strongly affected by the action of massive stars. They deposit in the ISM a huge number of ionizing photons and transfer to it vast amounts of mechanical energy via their powerful stellar winds. As a consequence, massive stars create what is known as an interstellar bubble, i.e., a minimum in the gas distribution characterized by a low volume density and a high temperature, surrounded by an expanding envelope (Weaver et al. 1977). The star should be seen projected onto, or close to, the centre of the H i minimum.

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

References

Münch, G. 1957, ApJ 125, 42.Google Scholar
Taylor, A.R. 2001, in: Clowes, R., Adamson, A. & Bromage, G. (eds.), The New Era of Wide Field Astronomy, ASP-CS 232, 235.Google Scholar
Walborn, N.R. 1971, ApJS 23, 257.Google Scholar
Weaver, R.P., McCray, R., Castor, J.I., Shapiro, P.R., Moore, R.L. 1977, ApJ 218, 377.Google Scholar