Single novae and interstellar accretion on white dwarfs

Details Single novae and interstellar accretion on white dwarfs Single novae and interstellar accretion on white dwarfs

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mmsai..50..179m&link_type=abstract

(Workshop on Chemical Inhomogeneities in the Galaxy, Frascati, Italy, May 29-June 2, 1978.) Società Astronomica Italiana, Memori

Astronomy and Astrophysics

Astronomy

Novae, Stellar Mass Accretion, White Dwarf Stars, Helium Hydrogen Atmospheres, Metals, Stellar Envelopes, Stellar Models

Scientific paper

The main possibilities of interstellar (i.s.) accretion on White Dwarfs (WDs) are investigated, in the light of the observations and of the more recent available data upon WDs envelope models. It is found that the upper limit to the i.s. accretion consistent with observations is approximately 9 orders of magnitude lower than the one requested for the existence of the so-called 'Single Novae', so that this last topic seems to be definitely ruled out.

Affiliated with

Also associated with

No associations

Rating

Single novae and interstellar accretion on white dwarfs 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 Single novae and interstellar accretion on white dwarfs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Single novae and interstellar accretion on white dwarfs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1653657