2008MNRAS.389.1414C


Query : 2008MNRAS.389.1414C

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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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 * gam Aql * 19 46 15.5789542266 +10 36 47.731401477 5.93 4.23 2.72 1.65 0.87 K3II 450 0
2 * bet Cep bC* 21 28 39.5968513 +70 33 38.574681 2.05 3.01 3.23 3.33 3.55 B0.5IIIs 756 0
3 * eps Peg LP* 21 44 11.1561394 +09 52 30.031152 5.61 3.91 2.39 1.34 0.58 K2Ib-II 464 1

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