Structural Peculiarities of Circumstellar Envelopes of the Young A0e Herbig Stars

Details Structural Peculiarities of Circumstellar Envelopes of the Young A0e Herbig Stars Structural Peculiarities of Circumstellar Envelopes of the Young A0e Herbig Stars

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..539p&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 539-540

Astronomy and Astrophysics

Astrophysics

3

Emission Line Profiles, Stellar Wind, Remote Shell, Inhomogeneity

Scientific paper

Circumstellar peculiarities of the A0-type Herbig stars are analyzed on the basis of high-resolution CCD spectroscopic data, obtained in 1991-1994 at the ESO and the Crimean Astrophysical Observatory (about 250 spectrograms). The results of investigation of the rapid line profile variability in Hα , Hβ , He I 5876 and DNa lines are presented for AB Aur, HD 163296, HD 36112 and HD 100546. The conclusion is made that the behaviour of these lines can be explained in the framework of the model containing an equatorially concentrated and azimuthally inhomogeneous stellar wind and an external cool shell occasionally losing matter in the form of infall on to the star.

Affiliated with

Also associated with

No associations

Rating

Structural Peculiarities of Circumstellar Envelopes of the Young A0e Herbig Stars 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 Structural Peculiarities of Circumstellar Envelopes of the Young A0e Herbig Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structural Peculiarities of Circumstellar Envelopes of the Young A0e Herbig Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1630449