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Soejima, Y; et al.
Originální název
Photometry of Three Superoutbursts of the SU UMa-Type Dwarf Nova, SW Ursae Majoris
Anglický název
Druh
Článek WoS
Originální abstrakt
We investigated superhump evolution, analysing optical photometric observations of the 2000 February-March, the 2002 October-November, and the 2006 September superoutbursts of SW UMa. The superhumps evolved in the same way after their appearance during the 2000 and 2002 superoutbursts, and probably during the 2006 one. This indicates that superhump evolution may be governed by invariable binary parameters. We detected a periodicity in the light curve after the end of the 2000 superoutburst without any phase shift, which seems to be the remains of the superhumps. We found QPOs at the end stage of the 2000 and 2002 superoutbursts, but failed to find extraordinarily large-amplitude QPOs, called 'super-QPOs', which previously had been observed in SW UMa.
Anglický abstrakt
Klíčová slova
QUASI-PERIODIC OSCILLATIONS; U-GEMINORUM STARS; VW HYDRI; WX CETI; CCD PHOTOMETRY; HV-VIRGINIS; X-RAY; SUPERHUMPS; MODEL; OUTBURSTS
Klíčová slova v angličtině
Autoři
Rok RIV
2011
Vydáno
25.08.2009
Nakladatel
Publ. Astron. Soc. Jpn
Místo
Tokyo
ISSN
0004-6264
Periodikum
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
Svazek
61
Číslo
4
Stát
Japonsko
Strany od
659
Strany do
674
Strany počet
15
BibTex
@article{BUT49459, author="Soejima, Y and et al.", title="Photometry of Three Superoutbursts of the SU UMa-Type Dwarf Nova, SW Ursae Majoris", journal="PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN", year="2009", volume="61", number="4", pages="659--674", issn="0004-6264" }