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Related papers: The Intriguing Polar EU Cancri in the Eyes of Kepl…

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We present time-resolved spectroscopic and polarimetric observations of the AM Her system EU Cnc. EU Cnc is located near the core of the old open cluster Messier 67; new proper motion measurements indicate that EU Cnc is indeed a member of…

Solar and Stellar Astrophysics · Physics 2013-04-01 Kurtis A. Williams , Steve B. Howell , James Liebert , Paul S. Smith , Andrea Bellini , Kate H. R. Rubin , Michael Bolte

We describe two observations of the nova-like cataclysmic variable AC Cnc obtained with {\it Kepler} during its revamped second mission ({\it K2}). Using the {\it K2} 1-minute cadence mode, the data were obtained during Campaigns 5 and 18.…

Solar and Stellar Astrophysics · Physics 2019-05-29 Eric M. Schlegel , R. Kent Honeycutt

On 2000 May 5, we began a large multi-wavelength campaign to study the intermediate polar, EX Hydrae. The simultaneous observations from six satellites and four telescopes were centered around a one million second observation with EUVE.…

Astrophysics · Physics 2009-11-07 Kunegunda E. Belle , Steve B. Howell , Martin Sirk , Mark E. Huber

Here we present the results of visible range light curve observations of ten Centaurs using the Kepler Space Telescope in the framework of the K2 mission. Well defined periodic light curves are obtained in six cases allowing us to derive…

We present simultaneous EUV and infrared (J,K) observations of the polar HU Aqr obtained during August 1998 when the star was in a high mass accretion state. EUV and IR light curves and EUV spectra are presented and compared with previous…

Astrophysics · Physics 2009-11-07 S. B. Howell , D. R. Ciardi , M. M. Sirk , A. D. Schwope

We report on the $XMM$-Newton observation of DW Cnc, a candidate intermediate polar candidate whose historical optical light curve shows the existence of periods at $\simeq 38$, $\simeq 86$ and $\simeq 69$ minutes which were interpreted as…

High Energy Astrophysical Phenomena · Physics 2019-01-23 A. A. Nucita , L. Conversi , D. Licchelli

CP Tuc (AX J2315--592) shows a dip in X-rays which lasts for approximately half the binary orbit and is deeper in soft X-rays compared with hard X-rays. It has been proposed that this dip is due to the accretion stream obscuring the…

Astrophysics · Physics 2009-10-31 Gavin Ramsay , Stephen Potter , David Buckley , Peter Wheatley

The K2 mission of the Kepler Space Telescope allowed the observations of light curves of small solar system bodies throughout the whole Solar system. In this paper we present the results of a collection of K2 transneptunian object…

Observations of Her X-1 by the Extreme Ultraviolet Explorer (EUVE) at the end of the x-ray Short High state are reported here. Her X-1 is found to exhibit a strong orbital modulation of the EUV flux, with a large dip superposed on a broad…

Astrophysics · Physics 2007-05-23 D. A. Leahy , H. Marshall

We carried out light curve solutions of two eclipsing detached binaries on eccentric orbits observed by Kepler. The orbits and fundamental parameters of KIC 11619964 and KIC 7118545 were determined with a high accuracy by modeling of their…

Solar and Stellar Astrophysics · Physics 2015-07-23 Diana Kjurkchieva , Doroteya Vasileva

We report the serendipituous discovery of the new eclipsing polar 2XMMp J131223.4+173659. Its striking X-ray light curve attracted immediate interest when we were visually inspecting the source products of the 2XMMp catalogue. This light…

Astrophysics · Physics 2009-11-13 J. Vogel , K. Byckling , A. Schwope , J. P. Osborne , R. Schwarz , M. G. Watson

With only two functional reaction wheels, Kepler cannot maintain stable pointing at its original target field and entered a new mode of observation called K2. Our method is based on many years of experience in planet hunting for the CoRoT…

Earth and Planetary Astrophysics · Physics 2016-10-19 S. C. C. Barros , O. Demangeon , M. Deleuil

Light curves of the Z Cam type dwarf nova AT Cnc observed during standstill in 2016 and 2018 are analyzed. On the time scale of hours, previous reports on periodicities, in particular the presence of negative superhumps, could not be…

Observations of Hercules X-1 by the Extreme Ultraviolet Explorer (EUVE) covering low state and the early part of the Short High state are reported here. This is the first EUV observation of this part of the 35-day cycle of Her X-1. The low…

Astrophysics · Physics 2009-10-31 D. A. Leahy , H. Marshall , D. Scott

We carried out light curve solutions of ten detached eclipsing eccentric binaries observed by Kepler. The formal errors of the derived parameters from the light curve solutions are below 1%. Our results give indications that the components…

Solar and Stellar Astrophysics · Physics 2016-05-25 D. Kjurkchieva , D. Vasileva

Observations of Neptune with the Kepler Space Telescope yield a 49-day light curve with 98% coverage at a 1-minute cadence. A significant signature in the light curve comes from discrete cloud features. We compare results extracted from the…

We report the detection of the polar CE Gru in X-rays for the first time. We find evidence for a dip seen in the hard X-ray light curve which we attribute to the accretion stream obscuring the accretion region in the lower hemisphere of the…

Astrophysics · Physics 2009-11-07 Gavin Ramsay , Mark Cropper

Context. The origin, evolution, and ultimate fate of magnetic cataclysmic variables are poorly understood. It is largely the nature of the magnetic fields in these systems that leads to this poor understanding. Fundamental properties, such…

Astrophysics of Galaxies · Physics 2009-11-13 O. W. Butters , S. Katajainen , A. J. Norton , H. J. Lehto , V. Piirola

We present simultaneous X-ray (lambda_peak ~ 44A) and EUV (lambda_peak = 89A) light curves for the magnetic cataclysmic variable QQ Vulpeculae, obtained with the EUVE satellite. We find that the unique shape of the X-ray light curve is…

Astrophysics · Physics 2009-10-31 Kunegunda E. Belle , Steve B. Howell , Amy Mills

We present phase-resolved XMM_Newton data of three short period polars: V347 Pav, GG Leo and EU UMa. All three systems show one dominant accretion region which is seen for approximately half of the orbital cycle. GG Leo shows a strong dip…

Astrophysics · Physics 2009-11-10 Gavin Ramsay , Mark Cropper , K. O. Mason , F. A. Cordova , W. Priedhorsky
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