Expected rate of neutrino bursts from collapsing stars in our Galaxy and the LMC

Details Expected rate of neutrino bursts from collapsing stars in our Galaxy and the LMC Expected rate of neutrino bursts from collapsing stars in our Galaxy and the LMC

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...190...69g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 190, no. 1-2, Jan. 1988, p. 69-71.

Astronomy and Astrophysics

Astrophysics

4

Magellanic Clouds, Milky Way Galaxy, Neutrinos, Supernova Remnants, Supernovae, Galactic Structure, Stellar Evolution, Supernova 1987A

Scientific paper

A spiral arms model of our Galaxy has been developed in order to estimate the rate of gravitational stellar collapses detectable at Earth. From the early optical observations and the neutrino signal of supernova 1987A, it is shown that most collapses in our Galaxy can be detected in neutrinos, even if the light outburst is too dim to be observed. The estimated rate of stellar collapses in the Large Magellanic Cloud, compared with the galactic one, seems to indicate a faster evolution in the LMC in comparison with our Galaxy.

Affiliated with

Also associated with

No associations

Rating

Expected rate of neutrino bursts from collapsing stars in our Galaxy and the LMC 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 Expected rate of neutrino bursts from collapsing stars in our Galaxy and the LMC, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Expected rate of neutrino bursts from collapsing stars in our Galaxy and the LMC will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1043492