Dynamics of Bubbles in the ISM

Details Dynamics of Bubbles in the ISM Dynamics of Bubbles in the ISM

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1156..285a&link_type=abstract

THE LOCAL BUBBLE AND BEYOND II: Proceedings of the International Conference. AIP Conference Proceedings, Volume 1156, pp. 285-2

Other

1

Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Supernova Remnants, Mass Loss And Stellar Winds, Masses, Cosmic Rays

Scientific paper

Bubbles are volumes of high temperature, low density gas surrounded by ionized and neutral shells. They form when hypersonic flows from massive stars interact with the interstellar medium. Other overpressured volumes of hot gas, such as supernova remnants and HII regions, can also be considered as bubbles. Simple analytical approximations exist to describe the expansion of these bubbles, however, meaningful comparisons with new observations can only be made if a more detailed, numerical approach is taken. In this paper, I describe some results of modeling these astrophysical objects.

Affiliated with

Also associated with

No associations

Rating

Dynamics of Bubbles in the ISM does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dynamics of Bubbles in the ISM, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of Bubbles in the ISM will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1313525