The ultraviolet spectrum of LSI + 61 deg 303

Details The ultraviolet spectrum of LSI + 61 deg 303 The ultraviolet spectrum of LSI + 61 deg 303

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..657h&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Oct.-Nov. 1979, p. 657, 658.

Astronomy and Astrophysics

Astronomy

9

B Stars, Radio Stars, Stellar Spectra, Ultraviolet Spectra, Variable Stars, Continuous Spectra, Gamma Ray Astronomy, Iue, Line Spectra, Spectral Energy Distribution, Supergiant Stars, X Ray Sources

Scientific paper

IUE spectroscopy is presented of the radio variable emission-line star LSI +61°303, which may also be a source of X and γ rays. The UV continuum is complex and dues nut fit a single stellar model or power law. The UV flux and line spectrum suggest the primary is a mass-losing Ib supergiant but all possibilities involve some peculiarities compared with normal stars. The spectrum appears to contain a very strong, variable N III feature at λ1750.

Affiliated with

Also associated with

No associations

Rating

The ultraviolet spectrum of LSI + 61 deg 303 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 The ultraviolet spectrum of LSI + 61 deg 303, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The ultraviolet spectrum of LSI + 61 deg 303 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1388517