Please use this identifier to cite or link to this item: https://www.um.edu.mt/library/oar/handle/123456789/96934
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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.authorBarrett, Dug-
dc.contributor.authorBoardman, James-
dc.contributor.authorBoyd, David-
dc.contributor.authorBrincat, Stephen M.-
dc.contributor.authorCarstens, Rolf-
dc.contributor.authorCollins, Donald F.-
dc.contributor.authorCook, Lewis M.-
dc.contributor.authorCooney, Walter R.-
dc.contributor.authorCejudo Fernández, David-
dc.contributor.authorDufoer, Sjoerd-
dc.contributor.authorDvorak, Shawn-
dc.contributor.authorGaldies, Charles-
dc.contributor.authorGoff, William-
dc.contributor.authorHambsch, Franz-Josef-
dc.contributor.authorJohnston, Steve-
dc.contributor.authorJones, Jim-
dc.contributor.authorMenzies, Kenneth-
dc.contributor.authorMonard, Libert A. G.-
dc.contributor.authorMorelle, Etienne-
dc.contributor.authorNelson, Peter-
dc.contributor.authorÖgmen, Yenal-
dc.contributor.authorRock, John W.-
dc.contributor.authorSabo, Richard-
dc.contributor.authorSeargeant, Jim-
dc.contributor.authorStone, Geoffrey-
dc.contributor.authorUlowetz, Joseph-
dc.contributor.authorVanmunster, Tonny-
dc.date.accessioned2022-06-02T06:46:53Z-
dc.date.available2022-06-02T06:46:53Z-
dc.date.issued2022-
dc.identifier.citationCovington, A. E., Shaw, A. W., Mukai, K., Littlefield, C., Heinke, C. O., Plotkin, R. M., ... & Vanmunster, T. (2022). Investigating the low-flux states in six Intermediate Polars. The Astrophysical Journal, 928(2), 164.en_GB
dc.identifier.urihttps://www.um.edu.mt/library/oar/handle/123456789/96934-
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 we 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_GB
dc.language.isoenen_GB
dc.publisherAmerican Astronomical Societyen_GB
dc.rightsinfo:eu-repo/semantics/openAccessen_GB
dc.subjectAstrophysicsen_GB
dc.subjectParticles (Nuclear physics)en_GB
dc.subjectPlasma dynamicsen_GB
dc.subjectX-ray astronomyen_GB
dc.subjectVariable starsen_GB
dc.subjectAccretion (Astrophysics)en_GB
dc.titleInvestigating the low-flux states in six intermediate polarsen_GB
dc.typearticleen_GB
dc.rights.holderThe copyright of this work belongs to the author(s)/publisher. The rights of this work are as defined by the appropriate Copyright Legislation or as modified by any successive legislation. Users may access this work and can make use of the information contained in accordance with the Copyright Legislation provided that the author must be properly acknowledged. Further distribution or reproduction in any format is prohibited without the prior permission of the copyright holder.en_GB
dc.description.reviewedpeer-revieweden_GB
dc.identifier.doi10.3847/1538-4357/ac5682-
dc.publication.titleThe Astrophysical Journalen_GB
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