A Spectroscopic Analysis of the γ Doradus Star HD 207223 = HR 8330

Details A Spectroscopic Analysis of the γ Doradus Star HD 207223 = HR 8330 A Spectroscopic Analysis of the γ Doradus Star HD 207223 = HR 8330

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...553..814a&link_type=abstract

The Astrophysical Journal, Volume 553, Issue 2, pp. 814-822.

Other

16

Stars: Individual (Hd 207223, Γ Doradus), Stars: Oscillations, Stars: Variables: Other

Scientific paper

We present a detailed analysis of 76 high-resolution, high signal-to-noise spectra of the γ Doradus star HD 207223=HR 8330. Periodogram analysis of the moments of the line profiles reveals a single period of 2.67+/-0.01 days, a result consistent with that found in photometric studies. Mode identification was accomplished with both the moment method and from direct line-profile fitting. Both methods clearly point towards a sectoral mode of degree l>=2. The inclusion of rotational effects, by taking the Coriolis force into account, reveals a single consistent solution: an l=m=+2 retrograde sectoral mode that has a period of 1.4 days in the corotating frame. The star is seen at an inclination of 30°. From this, we derive a rotational period of 4.9 days.

Affiliated with

Also associated with

No associations

Rating

A Spectroscopic Analysis of the γ Doradus Star HD 207223 = HR 8330 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 A Spectroscopic Analysis of the γ Doradus Star HD 207223 = HR 8330, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Spectroscopic Analysis of the γ Doradus Star HD 207223 = HR 8330 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1581899