SIMBAD references

1995A&A...299..707V - Astronomy and Astrophysics, volume 299, 707-714 (1995/7-3)

The multi-periodic pulsating PG 1159 white dwarf PG 0122+200.

VAUCLAIR G., PFEIFFER B., GRAUER A.D., BELMONTE J.A., JIMENEZ A., CHEVRETON M., DOLEZ N. and VIDAL I.

Abstract (from CDS):

PG 0122+200 is a hot pulsating PG 1159 [GW Virginis] star. This paper describes the results of two, bi-site, time-series photometric observational campaigns. The observed complex light curve is interpreted as resulting from a mixture of non radial g-mode pulsations. There appear to be at least ten independent frequencies in the power spectrum. The pulsation periods fall into four groups and are confined to a rather narrow interval between 336 and 470 seconds. The frequency resolution achieved (≃1.1µHz) reveals a fine structure which is interpreted as rotational splitting of l=1 modes. This splitting is consistent with a rotational period of 1.8 days for the star. We suspect that the observed modes are trapped modes separated by 3 or 4 undetected normal modes. Average period spacings of 16.70s or 16.16s are consistent with the data. However, a luminosity estimate and an irrefutable period spacing are necessary to determine PG 0122+200's mass.

Abstract Copyright:

Journal keyword(s): white dwarfs - stars: individual: PG 1159 (PG 1159-034) - stars: oscillations

CDS comments: RX J2117+3412 = RX J2117.1+3412

Simbad objects: 12

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2020.09.19-07:31:28

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