Detection of non-radial g-mode pulsations in the newly discovered PG 1159 star HE 1429-1209

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Detection of non - radial g - mode pulsations in the newly discovered PG 1159 star HE 1429 − 1209

We performed time-series photometry of the PG1159-type star HE 1429−1209, which was recently discovered in the ESO SPY survey. We show that the star is a low-amplitude (≈0.05 mag) non-radial g-mode pulsator with a period of 919 s. HE 1429−1209 is among the hottest known post-AGB stars (T eff =160 000 K) and, together with the known pulsator RX J2117.1+3412, it defines empirically the blue edge ...

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ژورنال

عنوان ژورنال: Astronomy & Astrophysics

سال: 2004

ISSN: 0004-6361,1432-0746

DOI: 10.1051/0004-6361:200400079