First results on the Be stars observed with the CoRoT satellite

Details First results on the Be stars observed with the CoRoT satellite First results on the Be stars observed with the CoRoT satellite

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.157...70g&link_type=abstract

Communications in Asteroseismology, Vol.157, p. 70-74

Computer Science

6

Scientific paper

In this paper we present an overview of the analysis of some of the Be stars observed with the CoRoT satellite up to this date. Be stars are very fast-rotating B-type stars which may pulsate as β Cephei or SPB stars. CoRoT has already observed 5 bright Be stars in the seismology fields and several tens of fainter ones in the exoplanet fields with an unprecedented quality and with a time duration from 20 to 150 days. Multiple frequencies are detected in the majority of the stars. Pulsations, outbursts, beating phenomenon, possible transient modes, rotation, amplitude variability, etc. have been found in their light curves. In order to complement this study, ground-based spectroscopic data have also been analysed for the stars located in the seismology fields.

Affiliated with

Also associated with

No associations

Rating

First results on the Be stars observed with the CoRoT satellite 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 First results on the Be stars observed with the CoRoT satellite, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and First results on the Be stars observed with the CoRoT satellite will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-964555