Supernovae in molecular clouds

Details Supernovae in molecular clouds Supernovae in molecular clouds

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...237..781w&link_type=abstract

Astrophysical Journal, Part 1, vol. 237, May 1, 1980, p. 781-792.

Astronomy and Astrophysics

Astrophysics

112

Interstellar Gas, Molecular Gases, Stellar Evolution, Supernova Remnants, Supernovae, Gas Density, Nebulae, Stellar Luminosity, Stellar Winds

Scientific paper

Similarity solutions are derived for the kinematic evolution of a supernova remnant buried in a molecular cloud of uniform density, and estimates are made for the emergent spectrum from the radio through the X-ray. The possible effects of density gradients in the cloud are considered. It is noted that the negative gradient prolongs the adiabatic phase and hence gives a higher luminosity at a given radius. The effects of a bubble blown by a stellar wind during the lifetime of the supernova star are outlined.

Affiliated with

Also associated with

No associations

Rating

Supernovae in molecular clouds 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 Supernovae in molecular clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernovae in molecular clouds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1358894