In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2
M. Gruberbauer - W.w. Weiss
Detaily:
Rok, strany: 2008, 311 - 316
Kľúčové slová:
stars: chemically peculiar, stars: oscillation, methods: observational, techniques: space photometry
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2008/Vol_38/No_2/pp311-316_abstract.html
O článku:
We discuss the potential of space photometry for rapidly oscillating Ap (roAp)
stars. In reference to the MOST observations of γ Equulei
(Gruberbauer et al., 2008), we show that several aspects of the roAp
phenomenon demand longer observational time bases and better time sampling
than those currently feasible using spectroscopy. We conclude that, in order
to improve our understanding of roAp stars, photometry is still an important
tool which should not be neglected.
Ako citovať:
ISO 690:
Gruberbauer, M., Weiss, W. 2008. On the benefits of photometry for roAp theory: MOST observations of γ Equulei (HD 201601). In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no.2, pp. 311-316. 1335-1842.
APA:
Gruberbauer, M., Weiss, W. (2008). On the benefits of photometry for roAp theory: MOST observations of γ Equulei (HD 201601). Contributions of the Astronomical Observatory Skalnaté Pleso, 38(2), 311-316. 1335-1842.