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Multi-epoch spectroscopy of IYUMa: quiescence, rise, normal outburst and superoutburst

Rolfe, D.J.; Haswell, Carole A.; Abbott, Timothy M.C.; Morales-Rueda, Luisa; Marsh, T.R. and Holdaway, G. (2005). Multi-epoch spectroscopy of IYUMa: quiescence, rise, normal outburst and superoutburst. Monthly Notices of the Royal Astronomical Society, 357(1) pp. 69–81.

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DOI (Digital Object Identifier) Link: https://doi.org/10.1111/j.1365-2966.2005.08639.x
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Abstract

We exploit rare observations covering the time before and during a normal outburst in the deeply eclipsing SUUMa system IYUMa to study the dramatic changes in the accretion flow and emission at the onset of outburst. Through Doppler tomography we study the emission distribution, revealing classic accretion flow behaviour in quiescence, with the stream-disc impact ionizing the nearby accretion disc. We observe a delay of hours to a couple of days between the rise in continuum and the rise in the emission lines at the onset of the outburst. From line profiles and Doppler maps during normal and superoutburst, we conclude that reprocessing of boundary layer (BL) radiation is the dominant emission line mechanism in outburst and that the normal outburst began in the outer disc. The stream-disc impact feature (the orbital hump) in the H? line flux light curve disappears before the onset of the normal outburst and may be an observable signal heralding an impending outburst.

Item Type: Journal Item
ISSN: 1365-2966
Keywords: techniques: spectroscopic, stars: dwarf novae, stars: individual: IYUMa, novae, cataclysmic variables
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 11287
Depositing User: Astrid Peterkin
Date Deposited: 08 Aug 2008 09:17
Last Modified: 12 Dec 2018 18:35
URI: http://oro.open.ac.uk/id/eprint/11287
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