Investigating the Low-flux States in Six Intermediate Polars

Author:

Covington Ava E.,Shaw Aarran W.ORCID,Mukai KojiORCID,Littlefield ColinORCID,Heinke Craig O.ORCID,Plotkin Richard M.ORCID,Barrett Doug,Boardman James,Boyd David,Brincat Stephen M.,Carstens Rolf,Collins Donald F.,Cook Lewis M.,Cooney Walter R.,Fernández David Cejudo,Dufoer Sjoerd,Dvorak Shawn,Galdies Charles,Goff William,Hambsch Franz-Josef,Johnston Steve,Jones Jim,Menzies Kenneth,Monard Libert A. G.,Morelle Etienne,Nelson Peter,Ögmen Yenal,Rock John W.,Sabo Richard,Seargeant Jim,Stone Geoffrey,Ulowetz Joseph,Vanmunster Tonny

Abstract

Abstract We 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.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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