SIMBAD references

2008MNRAS.389.1414C - Mon. Not. R. Astron. Soc., 389, 1414-1418 (2008/September-3)

The spectroscopic variability of Teff and logg in the hot pulsating star βCephei.

CATANZARO G. and LEONE F.

Abstract (from CDS):

Time resolved spectra of βCep yield the following average results: Teff= 24000±250 K, logg = 3.91±0.05 and ξ = 8.1±0.9 km/s. Nitrogen, oxygen, neon, aluminium, silicon and sulfur abundances are solar while carbon, magnesium and iron are slightly underabundant. Pulsational amplitudes of ΔTeff∼ 700 K and Δlogg ∼ 0.2 dex are found from Hβ. The metal lines give similar amplitudes but centred on Teff∼ 25000 K. An upper limit of 1.0 km/s to the variability of the microturbulence is derived from the Siiii triplet at 455 nm. The radial-velocity amplitude derived from the core of Hβ is ∼15 per cent greater than that from the metal lines.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): stars: abundances - stars: early-type - stars: individual: β Cephei - stars: oscillations

Simbad objects: 3

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