The UV resonance lines of Zeta-1 SCO

Details The UV resonance lines of Zeta-1 SCO The UV resonance lines of Zeta-1 SCO

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....78...15w&link_type=abstract

Astronomy and Astrophysics, vol. 78, no. 1, Sept. 1979, p. 15-20. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astronomy

17

Line Spectra, Stellar Spectra, Supergiant Stars, Ultraviolet Astronomy, Absorption Spectra, B Stars, Iue, Stellar Envelopes, Stellar Mass Ejection

Scientific paper

The IUE satellite has been used to obtain high-resolution UV spectrograms of the extreme B1 supergiant Zeta-1 Sco. The observed line spectrum was found to be dominated by conspicuous P Cygni profiles or strongly blueshifted circumstellar absorption lines of the resonance transitions of Al II, Mg II, Si II, C II, Al III, Si IV, C IV, and N V, and of Fe III multiplets originating from metastable lower states. The observed line profiles are compared with different models of the velocity field and ionization structure of the expanding envelope of Zeta-1 Sco.

Affiliated with

Also associated with

No associations

Rating

The UV resonance lines of Zeta-1 SCO 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 UV resonance lines of Zeta-1 SCO, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The UV resonance lines of Zeta-1 SCO will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1817238