Investigating the low-flux states in six Intermediate Polars

dc.contributor.authorCovington, Ava E.
dc.contributor.authorShaw, Aarran W.
dc.contributor.authorMukai, Koji
dc.contributor.authorLittlefield, Colin
dc.contributor.authorHeinke, Craig O.
dc.contributor.authorPlotkin, Richard M.
dc.contributor.authoret al
dc.date.accessioned2022-03-29T16:38:49Z
dc.date.available2022-03-29T16:38:49Z
dc.date.issued2022-02-19
dc.descriptionAva E. Covington, Aarran W. Shaw, Koji Mukai, Colin Littlefield, Craig O. Heinke, Richard M. Plotkin, Doug Barrett, James Boardman, David Boyd, Stephen M. Brincat, Rolf Carstens, Donald F. Collins, Lewis M. Cook, Walter R. Cooney, David Cejudo Fernández, Sjoerd Dufoer, Shawn Dvorak, Charles Galdies, William Goff, Franz-Josef Hambsch, Steve Johnston, Jim Jones, Kenneth Menzies, Libert A. G. Monard, Etienne Morelle, Peter Nelson, Yenal Öğmen, John W. Rock, Richard Sabo, Jim Seargeant, Geoffrey Stone, Joseph Ulowetz, Tonny Vanmunsteren_US
dc.description.abstractWe present optical photometry of six intermediate polars that exhibit transitions to a low-flux state. For four of these systems, DW Cnc, V515 And, V1223 Sgr and RX J2133.7+5107, we are able to perform timing analysis in and out of the low states. We find that, for DW Cnc and V515 And, the dominant periodicities in the light curves change as the flux decreases, indicating a change in the sources' accretion properties as they transition to the low state. For V1223 Sgr we find that the variability is almost completely quenched at the lowest flux, but do not find evidence for a changing accretion geometry. For RX J2133.7+5107, the temporal properties do not change in the low state, but we do see a period of enhanced accretion that is coincident with increased variability on the beat frequency, which we do not associate with a change in the accretion mechanisms in the system.en_US
dc.description.sponsorshipThe authors thank the anonymous referee for com ments that helped improve the manuscript. AEC ac knowledges partial support from the Nevada Under graduate Research Award. AWS thanks Jean-Marie Hameury for fruitful discussions on the outbursts in V1223 Sgr. We acknowledge with thanks the vari able star observations from the AAVSO International Database contributed by observers worldwide and used in this research. AWS thanks Elizabeth Waagen of the AAVSO for facilitating the inclusion of AAVSO ob servers as co-authorsen_US
dc.description.urihttps://arxiv.org/abs/2202.08365en_US
dc.format.extent19 pagesen_US
dc.genrejournal articlesen_US
dc.genrepreprintsen_US
dc.identifierdoi:10.13016/m2hwqe-o1k6
dc.identifier.urihttps://doi.org/10.48550/arXiv.2202.08365
dc.identifier.urihttp://hdl.handle.net/11603/24453
dc.language.isoen_USen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Faculty Collection
dc.relation.ispartofUMBC Physics Department
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en_US
dc.titleInvestigating the low-flux states in six Intermediate Polarsen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-8286-8094en_US

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