Diameter distribution and Sigma-D relation of SNRs in M31 and M33

Details Diameter distribution and Sigma-D relation of SNRs in M31 and M33 Diameter distribution and Sigma-D relation of SNRs in M31 and M33

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...120..147b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 120, no. 1, April 1983, p. 147-149.

Astronomy and Astrophysics

Astrophysics

13

Andromeda Galaxy, Brightness, Diameters, Size Distribution, Spiral Galaxies, Supernova Remnants, Adiabatic Conditions, Milky Way Galaxy, Spatial Distribution, Surface Properties

Scientific paper

The diameter distribution relations for SNRs in M31 and M33 are considerably flatter than expected for SNRs in their adiabatic expansion phase. Surface brightness-diameter relations for these objects are, however, consistent with the relation for SNRs in the Galaxy. If only the most luminous SNRs have been detected so far, the intrinsic luminosity spread becomes more than a factor of 10.

Affiliated with

Also associated with

No associations

Rating

Diameter distribution and Sigma-D relation of SNRs in M31 and M33 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 Diameter distribution and Sigma-D relation of SNRs in M31 and M33, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Diameter distribution and Sigma-D relation of SNRs in M31 and M33 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1232960