Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...323..505b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 323, Dec. 15, 1987, p. 505-515.
Astronomy and Astrophysics
Astronomy
55
Galactic Nuclei, Irregular Galaxies, Radio Sources (Astronomy), Star Formation, Supernovae, Astronomical Models, Astronomical Photometry, Very Long Base Interferometry
Scientific paper
The authors have used the Mark III VLBI system to observe, at 2.3 and 8.4 GHz simultaneously, 23 hot spots in the nuclear region of the nearby starburst galaxy M82. The authors detected six hot spots at 2.3 GHz but only one at 8.4 GHz. The brightness distribution and an upper limit on the expansion rate of the brightest hot spot, 41.9+58, is derived. These results and the diameters and ages, or corresponding lower bounds, for 13 more hot spots are consistent with the hot spots in M82 being powerful supernova remnants with ages between ≡10 and ≡300 yr. The authors estimate a radio supernova rate of ≡0.1 yr-1 for the inner 600 pc of M82.
Bartel Norbert
Bonometti R. J.
Cohen Norman L.
Gorenstein M. V.
Marcaide Juan Maria
No associations
LandOfFree
VLBI observations of 23 hot spots in the starburst 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 VLBI observations of 23 hot spots in the starburst galaxy M82, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLBI observations of 23 hot spots in the starburst galaxy M82 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-901170