Pre-existing dust shells around type-I supernovae

Details Pre-existing dust shells around type-I supernovae Pre-existing dust shells around type-I supernovae

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111..419p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 2, April 1985, p. 419-424.

Astronomy and Astrophysics

Astronomy

1

Cosmic Dust, Infrared Astronomy, R Coronae Borealis Stars, Stellar Envelopes, Stellar Evolution, Supernovae, Carbon Stars, Dwarf Novae, Stellar Models

Scientific paper

The possibility of the existence, around type-I supernovae, of dust shells which existed before a supernova outburst is considered. None have so far been detected observationally; and any dust around the progenitor radiating in the near infrared would evaporate at outburst. Far infrared observations of the two possible types of progenitor, R Coronae Borealis-type stars and dwarf novae, would be useful to indicate whether there is any dust around them which would survive a supernova outburst.

Affiliated with

Also associated with

No associations

Rating

Pre-existing dust shells around type-I supernovae 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 Pre-existing dust shells around type-I supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pre-existing dust shells around type-I supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1288512