IUE observations of CH Cygni continuum during 1979-1986

Details IUE observations of CH Cygni continuum during 1979-1986 IUE observations of CH Cygni continuum during 1979-1986

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.131..725m&link_type=abstract

(IAU, Colloquium on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, 93rd, Bamberg, West

Astronomy and Astrophysics

Astronomy

10

Binary Stars, Cataclysmic Variables, Continuous Spectra, Spectrum Analysis, Stellar Spectrophotometry, Ultraviolet Spectra, Atmospheric Temperature, Iue, Spaceborne Astronomy, Spectral Energy Distribution, Stellar Models

Scientific paper

Variations of the UV continuum have been analyzed. The observed UV continuum may be reproduced by a superposition of a Kurucz model atmosphere (log g = 2), Teff ≡ 8500 - 15000K) and optically thin hydrogen bound-free and free-free emission (Te ≡ 1000K). The temperature of the Kurucz atmosphere is the lowest at the maximum of brightness. The flat minimum in the UV integrated flux was observed in May - October 1985.

Affiliated with

Also associated with

No associations

Rating

IUE observations of CH Cygni continuum during 1979-1986 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 IUE observations of CH Cygni continuum during 1979-1986, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and IUE observations of CH Cygni continuum during 1979-1986 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1452638