SIMBAD references

2003MNRAS.345.1266W - Mon. Not. R. Astron. Soc., 345, 1266-1270 (2003/November-2)

The new AM CVn star in Hydra.

WOUDT P.A. and WARNER B.

Abstract (from CDS):

High-speed photometry of the new AM CVn star in Hya (previously known as SN2003aw), spectroscopically identified by Chornock & Filippenko, shows it to have a superhump period of 2041.5±0.3 s. We find a range of brightness from V ∼ 16.5 to 20.3, presumably caused by variations in the rate of mass transfer. In the intermediate state the system cycles in brightness with a period of ∼16 h and range ≥0.4 mag. There are sidebands to the principal frequencies in the Fourier transform which have constant frequency difference from the superhump harmonics.

Abstract Copyright: 2003 RAS

Journal keyword(s): techniques: photometric - binaries: close - stars: individual: 2003aw - novae, cataclysmic variables

Simbad objects: 13

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2021.05.16-19:55:06

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