The Power Problem in Superbubbles

Details The Power Problem in Superbubbles The Power Problem in Superbubbles

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1156..295o&link_type=abstract

THE LOCAL BUBBLE AND BEYOND II: Proceedings of the International Conference. AIP Conference Proceedings, Volume 1156, pp. 295-3

Physics

1

Mass Loss And Stellar Winds, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Supernovae, Cosmic Rays, X-Ray Sources, X-Ray Bursts

Scientific paper

The Local Bubble is generally presumed to be a hot superbubble generated by stellar winds and supernovae. Superbubbles are common in star-forming galaxies, and while their origin from massive star feedback is generally accepted, their dominant physical processes and evolution still remain to be quantitatively confirmed. This paper reviews the status of our understanding on the most important issue, the energy budget for superbubbles.

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