Towards asteroseismology of the non-radial pulsating sdB star PG 1605+072

Details Towards asteroseismology of the non-radial pulsating sdB star PG 1605+072 Towards asteroseismology of the non-radial pulsating sdB star PG 1605+072

2002-12-20

arxiv.org/abs/astro-ph/0212489v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, Proc. XIII Workshop on White Dwarfs, eds. D. de Martino, R. Kalytis, R. Silvotti, J.E. Solheim, Kluwer

Scientific paper

The recently discovered new class of sdB pulsators (sdBV) offers a powerful possibility for the investigation of their interior and thus their evolutionary history. The first step towards applying asteroseismologic tools is the identification of pulsation modes. We reoport on simultaneous spectroscopic and multi-band photometric time series observations of PG 1605+072 and analyse its radial velocity and light curve.

Affiliated with

Also associated with

No associations

Rating

Towards asteroseismology of the non-radial pulsating sdB star PG 1605+072 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 Towards asteroseismology of the non-radial pulsating sdB star PG 1605+072, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Towards asteroseismology of the non-radial pulsating sdB star PG 1605+072 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-724452