Quasi-molecular satellites of Lyman beta in ORFEUS observations of DA white dwarfs

Details Quasi-molecular satellites of Lyman beta in ORFEUS observations of DA white dwarfs Quasi-molecular satellites of Lyman beta in ORFEUS observations of DA white dwarfs

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...336..276k&link_type=abstract

Astronomy and Astrophysics, v.336, p.276-280 (1998)

Astronomy and Astrophysics

Astrophysics

19

Stars: White Dwarfs, Stars: Atmospheres, Ultraviolet: Stars, Line: Profiles

Scientific paper

Quasi-molecular satellite features of Ly beta were first observed in a HUT spectrum of the DA white dwarf Wolf 1346 and interpreted by Koester et al. (1996). In this paper we study the dependence of these features on temperature and surface gravity in 4 additional DA observed with ORFEUS-SPAS II in 1996. For the interpretation we use theoretical atmosphere models which incorporate new profiles for Ly beta . These have been calculated by Allard et al. (1998a) including the variation of the transition probability with distance between emitter and perturber. The new calculations for the general line shape, satellite positions and strengths are in very good agreement with the observations.

Affiliated with

Also associated with

No associations

Rating

Quasi-molecular satellites of Lyman beta in ORFEUS observations of DA white dwarfs 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 Quasi-molecular satellites of Lyman beta in ORFEUS observations of DA white dwarfs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quasi-molecular satellites of Lyman beta in ORFEUS observations of DA white dwarfs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1573611