Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009apj...693l..16s&link_type=abstract
The Astrophysical Journal Letters, Volume 693, Issue 1, pp. L16-L18 (2009).
Astronomy and Astrophysics
Astronomy
5
Accretion, Accretion Disks, Novae, Cataclysmic Variables, Stars: Individual: Dq Her, Stars: Oscillations: Including Pulsations
Scientific paper
We report an eclipse-mapping analysis of the 71 s pulsation of DQ Her in the He II λ4686 line. The observed pulse phase-dependent illumination pattern can be explained in terms of an asymmetric oblique dipole accretor model, in which X-ray beams from the accretion poles are reprocessed in two arched accretion curtains and in a vertically extended bright spot (BS) of half-thickness H = (7.4 ± 0.4) × 10-3 R sun at the disk rim. The optical pulsation is dominated by reprocessing at the BS, indicating that the 71 s pulsation is the beat period between the white dwarf (WD) spin (P spin = 70.8 s) and the orbital period. Our results exclude the possibility that the rotation period of the WD is 142 s.
Baptista Raymundo
Saito Roberto K.
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