AB Aurigae and its variable hydrogen lines

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12

B Stars, Stellar Envelopes, Stellar Spectra, Variable Stars, Balmer Series, Hydrogen, Line Spectra, Main Sequence Stars, Radial Velocity, Stellar Winds

Scientific paper

Coudé spectrograms of dispersion 8 and 16 Å/mm of the variable Herbig Ae/Be star AB Aur are discussed. The material was obtained on 8 different nights between 1970 and 1981 and covers the range 3450-4950 Å. From this material and a 5.3 Å/mm echelle spectrogram of Hα and NaD a stellar wind, possibly decelerated, and a relatively compact emitting region close to the star is suggested. The later region is variable on time scales of less than a day. The heliocentric radial velocity of AB Aur of +21±10 km s-1 is in agreement with +15.3±0.6 km s-1 observed for the associated molecular cloud. The possibility that AB Aur is a member in a close binary system is not supported.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

AB Aurigae and its variable hydrogen lines 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 AB Aurigae and its variable hydrogen lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and AB Aurigae and its variable hydrogen lines will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-741137

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.