SIMBAD references

2005A&A...441..231Q - Astronomy and Astrophysics, volume 441, 231 (2005/10-1)

The nature of the driving mechanism in the pulsating hybrid PG 1159 star Abell 43.

QUIRION P.-O., FONTAINE G. and BRASSARD P.

Abstract (from CDS):

We extend our previous pulsational stability analyses of PG 1159 stars by modeling the hybrid PG 1159 type star Abell 43. We show that the standard κ-mechanism due to the ionization of C and O in the envelope of this H-rich PG 1159 star is perfectly able to drive g-mode pulsations. Thus, contrary to a recent suggestion, there is no need to invoke any new or exotic mechanism to explain the pulsational instabilities observed in this particular star. Our expected instability band for l=1 modes extends in period from ∼2604s to ∼5529s, which is consistent with the available photometric observations of Abell 43. We also suggest that efforts to detect luminosity variations in its sibling NGC 7094 be pursued.

Abstract Copyright:

Journal keyword(s): stars: white dwarfs - stars: oscillations - stars: individual: Abell 43

Simbad objects: 4

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2019.12.05-16:24:24

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