Photometric and Spectroscopic Monitoring of the sdBV star PG 1605+072: The Multi-Site Spectroscopic Telescope (MSST) Project

Simple item page
dc.creatorHeber, U.
dc.creatorDreizler, S.
dc.creatorSchuh, S. L.
dc.creatorO'Toole, S.
dc.creatorJeffery, C. S.
dc.date2002-12-19
dc.date.accessioned2026-07-07T02:06:57Z
dc.date.available2026-07-07T02:06:57Z
dc.descriptionA 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.
dc.description4 pages, no figures, Proc. XIII Workshop on White Dwarfs, eds. D. de Martino, R. Kalytis, R. Silvotti, J.E. Solheim, Kluwer
dc.identifierhttps://arxiv.org/abs/astro-ph/0212447
dc.identifierhttp://arxiv.org/abs/astro-ph/0212447
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5540
dc.subjectAstrophysics
dc.titlePhotometric and Spectroscopic Monitoring of the sdBV star PG 1605+072: The Multi-Site Spectroscopic Telescope (MSST) Project
dc.typetext

Files

Collections

arXiv