Spectroscopic mode identification of main-sequence non-radially pulsating stars

Details Spectroscopic mode identification of main-sequence non-radially pulsating stars Spectroscopic mode identification of main-sequence non-radially pulsating stars

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.328..105m&link_type=abstract

Astrophysics and Space Science, Volume 328, Issue 1-2, pp. 105-108

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We are undertaking an extensive observational campaign of a number of non-radially pulsating stars using the high-resolution HERCULES spectrograph on the 1.0-m telescope at the Mt John University Observatory. This is part of a large world-wide multi-site campaign to improve mode-identification techniques in non-radially pulsating stars, particularly for g-mode pulsators. This paper outlines our campaign and presents preliminary results for one γ Doradus star, HD 40745, and one β Cephei star, HD 61068. We have used a representative cross-correlation line-profile technique presented by Wright in 2008 to extract line profiles and these have then been analyzed using the FAMIAS package due to Zima published in 2006 to derive a spectroscopic mode identification.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic mode identification of main-sequence non-radially pulsating 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 Spectroscopic mode identification of main-sequence non-radially pulsating stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic mode identification of main-sequence non-radially pulsating stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1645756