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Dwarf Novae in the OGLE Data. II. Forty New Dwarf Novae in the OGLE-III Galactic Disk Fields

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arxiv 1307.1238 v2 pith:LWUPIZCF submitted 2013-07-04 astro-ph.GA astro-ph.SR

classification astro-ph.GAastro-ph.SR
keywords typestarsdwarfnovaeobjectsogle-iiioutburstssuperoutbursts
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We report the discovery of forty erupting cataclysmic variable stars in the OGLE-III Galactic disk fields: seventeen objects of U Gem type, four of Z Cam type, and nineteen stars showing outbursts and superoutbursts typical for SU UMa type dwarf novae. In the case of five stars we were able to estimate their supercycle lengths. The obtained lengths are in the range 20-90 d, generally between the typical SU UMa type variables and a few objects classified as the ER UMa type variables. Since there is no significant difference between the two types but a higher mass-transfer rate resulting in more frequent outbursts and superoutbursts in the ER UMa type stars, we propose to discard this type as a separate class of variables. We note that in one of the SU UMa type stars, OGLE-GD-DN-039, we found a negative supercycle period change, in contrast to other active systems of this type. Two of the new OGLE objects showed long-duration WZ Sge-like superoutbursts followed by a sequence of echo outbursts. All stars reported in this paper are part of the OGLE-III Catalog of Variable Stars.

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  1. The S-PLUS 12-band photometry as a powerful tool for discovery and classification: ten cataclysmic variables in a proof-of-concept study

    astro-ph.SR 2025-01 conditional novelty 6.0 of 10

    A proof-of-concept that S-PLUS 12-band photometric colors and SED shape can select cataclysmic variables, with 10 systems confirmed by spectroscopy.

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