Implications of the UV observations of SN 1987 A

Details Implications of the UV observations of SN 1987 A Implications of the UV observations of SN 1987 A

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...177l..33f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 177, no. 1-2, May 1987, p. L33-L36.

Astronomy and Astrophysics

Astrophysics

36

Interstellar Matter, Supernova 1987A, Ultraviolet Spectra, Absorption Spectra, Line Spectra, Neutrinos, Stellar Atmospheres, White Dwarf Stars

Scientific paper

The implications of the UV observations of SN 1987A are discussed. The authors conclude that the UV spectrum is not a distinguishing feature between Type I and II supernovae. There is therefore no contradiction with the optical observations. Instead it is proposed that the differences in the UV properties are to be sought in the varying degree of interaction with the circumstellar environment. It is also shown that the absence of N V 1238 - 43 in the absorption line spectrum gives a stringent limit on the energy in the very early EUV burst expected from the supernova.

Affiliated with

Also associated with

No associations

Rating

Implications of the UV observations of SN 1987 A 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 Implications of the UV observations of SN 1987 A, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Implications of the UV observations of SN 1987 A will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-856020