Ultraviolet observations of a Bp-star at high galactic latitude

Details Ultraviolet observations of a Bp-star at high galactic latitude Ultraviolet observations of a Bp-star at high galactic latitude

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157...29b&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

2

Hot Stars, Iue, Magnesium, Ultraviolet Astronomy, Absorption Spectra, Doppler Effect, Extraterrestrial Radiation, High Speed, Interstellar Matter, Radial Velocity, Stellar Atmospheres

Scientific paper

The high velocity metal-poor star HD 214 539 AOIB was analyzed for Mg II lines around 2800 A. It was possible to separate the interstellar components. According to predicted and observed correlation between the Mg II UV lines in supergiants as a function of spectral type of effective temperature, the predicted Mg II line intensity is at least 1 A. This suggests a great underabundance of Mg II in HD 214 539.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet observations of a Bp-star at high galactic latitude 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 Ultraviolet observations of a Bp-star at high galactic latitude, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet observations of a Bp-star at high galactic latitude will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1698201