Photometric and Spectroscopic Monitoring of the sdBV star PG 1605+072: The Multi-Site Spectroscopic Telescope (MSST) Project
Abstract
A small fraction of subluminous B stars show short-period, multiperiodic light variations and form the new class of pulsating star known as EC 14026 variables, after the prototype. The Multi-Site Spectroscopic Telescope (MSST) is a virtual instrument and is also the name of a collaboration that aims to open up a new observational window to provide access to a mode identification for and an asteroseismological analysis of the pulsating sdB star PG 1605+072. Although the primary aim is to obtain time resolved spectroscopy it also includes the most extended photometric monitoring campaign for PG 1605+072.
- Publication:
-
White Dwarfs
- Pub Date:
- 2003
- DOI:
- 10.1007/978-94-010-0215-8_32
- arXiv:
- arXiv:astro-ph/0212447
- Bibcode:
- 2003ASIB..105..105H
- Keywords:
-
- Astrophysics
- E-Print:
- 4 pages, no figures, Proc. XIII Workshop on White Dwarfs, eds. D. de Martino, R. Kalytis, R. Silvotti, J.E. Solheim, Kluwer