HM Sagittae - The evolution of a symbiotic nova

Details HM Sagittae - The evolution of a symbiotic nova HM Sagittae - The evolution of a symbiotic nova

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...236..117n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 236, no. 1, Sept. 1990, p. 117-132. Research supported by SNSF.

Statistics

Computation

39

Binary Stars, Novae, Stellar Evolution, Stellar Mass Accretion, Stellar Radiation, Symbiotic Stars, Ultraviolet Radiation, Astronomical Spectroscopy, Computational Astrophysics, Iue, Sagittarius Constellation, Stellar Luminosity, Stellar Models

Scientific paper

HM Sge was discovered in 1975, when it became a symbiotic nova. HM Sge is still evolving. Since its discovery, significant spectral changes have taken place in the ultraviolet, the radio, as well as in the visual wavelength ranges. Here, IUE observations from 1982 to 1989 are reported. The implications of the available spectral information since the outburst in 1975 are then discussed.

Affiliated with

Also associated with

No associations

Rating

HM Sagittae - The evolution of a symbiotic nova 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 HM Sagittae - The evolution of a symbiotic nova, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HM Sagittae - The evolution of a symbiotic nova will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1399769