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Phase-resolved spectroscopy of the helium dwarf nova 'SN 2003aw' in quiescence

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Roelofs, Gijs H. A., Groot, P. J. (Paul J.), Marsh, T. R., Steeghs, D. (Danny), 1972- and Nelemans, G.. (2006) Phase-resolved spectroscopy of the helium dwarf nova 'SN 2003aw' in quiescence. Monthly Notices of the Royal Astronomical Society, Vol.365 (No.4). pp. 1109-1113. ISSN 0035-8711

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Official URL: http://dx.doi.org/10.1111/j.1365-2966.2005.09727.x

Abstract

High time resolution spectroscopic observations of the ultracompact helium dwarf nova 'SN 2003aw' in its quiescent state at V similar to 20.5 reveal its orbital period at 2027.8 +/- 0.5 s or 33.80 min. Together with the photometric 'superhump' period of 2041.5 +/- 0.5 s, this implies a mass ratio q approximate to 0.036. We compare both the average and time-resolved spectra of 'SN 2003aw' and Sloan Digital Sky Survey (SDSS) J124058.03-015919.2. Both show a DB white dwarf spectrum plus an optically thin, helium-dominated accretion disc. 'SN 2003aw' distinguishes itself from the SDSS source by its strong calcium H & K emission lines, suggesting higher abundances of heavy metals than the SDSS source. The silicon and iron emission lines observed in the SDSS source are about twice as strong in 'SN 2003aw'. The peculiar 'double bright spot' accretion disc feature seen in the SDSS source is also present in time-resolved spectra of 'SN 2003aw', albeit much weaker.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Dwarf novae, Cataclysmic variable stars
Journal or Publication Title: Monthly Notices of the Royal Astronomical Society
Publisher: Wiley-Blackwell Publishing, Inc
ISSN: 0035-8711
Date: 1 February 2006
Volume: Vol.365
Number: No.4
Number of Pages: 5
Page Range: pp. 1109-1113
Identification Number: 10.1111/j.1365-2966.2005.09727.x
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Funder: Nederlandse Organisatie voor Wetenschappelijk Onderzoek [Netherlands Organisation for Scientific Research] (NWO), Smithsonian Astrophysical Observatory, Particle Physics and Astronomy Research Council (Great Britain) (PPARC)
Grant number: 639.042.201 (NWO), 639.041.405 (NWO)
References: Anderson S. F. et al., 2005, AJ, submitted (astro-ph/0506730) Chornock R., Filippenko A. V., 2003, IAUC, 8084 Marsh T. R., Horne K., 1988, MNRAS, 235, 269 Marsh T. R., Horne K., Rosen S., 1991, ApJ, 366, 535 Nather R. E., Robinson E. L., Stover R. J., 1981, ApJ, 224, 269 Nelemans G., 2005, ASPC, 330, 27 (astro-ph/0409676) Nelemans G., Steeghs D., Groot P. J., 2001, MNRAS, 326, 621 Nogami D., Monard B., Retter A., Liu A., Uemura M., Ishioka R., Imada A., Kato T., 2004, PASJ, 56L, 39 Patterson J. et al., 2005, PASP, in press (astro-ph/0507371) Roelofs G. H. A., Groot P. J., Marsh T. R., Steeghs D., Barros S. C. C, Nelemans G., 2005, MNRAS, 361, 487 Wood-Vasey W. M., Aldering G., Nugent P., Li K., 2003, IAUC, 8077 Woudt P. A., Warner B., 2003, MNRAS, 345, 1266 Woudt P. A., Warner B., 2005, IAUC, 8531
URI: http://wrap.warwick.ac.uk/id/eprint/33932

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