Young supernovae in the starbust galaxy M82

Details Young supernovae in the starbust galaxy M82 Young supernovae in the starbust galaxy M82

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..783u&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Dec. 15, 1984, p. 783-792.

Astronomy and Astrophysics

Astronomy

43

Radio Galaxies, Radio Sources (Astronomy), Stellar Evolution, Supernova Remnants, Supernovae, Astronomical Photography, Radiant Flux Density, Radio Astronomy, Starburst Galaxies

Scientific paper

MERLIN observations at frequencies of 408, 1666 and 4995 MHz reveal 18 compact (less than 0.25 arcsec) radio sources within the central few hundred parsecs of M82. M82 is well known as a 'starburst' galaxy, and it is probable that these objects are either radio supernovae or young supernova remnants. The distribution of radio sources appears asymmetric with respect to the centre of the galaxy, and it is suggested that this is due to the current region of star formation lying within a molecular ring.

Affiliated with

Also associated with

No associations

Rating

Young supernovae in the starbust galaxy M82 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 Young supernovae in the starbust galaxy M82, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Young supernovae in the starbust galaxy M82 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-738080