1![Faint Cataclysmic Variables in the ! globular cluster 47 Tucanae *Rivera Sandoval L.E.1; van den Berg, M.1,2; Heinke, C. O.3; Cool, A.4; Cohn, H. N.5; Lugger, P. M.5 ; Ivanova N.3; Edmonds P.D.4; Grindlay J.E. 2 Faint Cataclysmic Variables in the ! globular cluster 47 Tucanae *Rivera Sandoval L.E.1; van den Berg, M.1,2; Heinke, C. O.3; Cool, A.4; Cohn, H. N.5; Lugger, P. M.5 ; Ivanova N.3; Edmonds P.D.4; Grindlay J.E. 2](https://www.pdfsearch.io/img/e79c284574d83017156e6a317b658f51.jpg) | Add to Reading ListSource URL: cxc.cfa.harvard.eduLanguage: English - Date: 2014-12-23 09:41:27
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2![No.32 OctISSN No.32 OctISSN](https://www.pdfsearch.io/img/21f4772c900f0df77d969aafbe97ce21.jpg) | Add to Reading ListSource URL: vsolj.cetus-net.orgLanguage: English - Date: 2004-02-05 23:12:08
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3![The Astrophysical Journal, 755:158 (8pp), 2012 August 20 Cdoi:637X The Astrophysical Journal, 755:158 (8pp), 2012 August 20 Cdoi:637X](https://www.pdfsearch.io/img/809717e4487ebcdec4869067feb99e58.jpg) | Add to Reading ListSource URL: schwab.tsuniv.eduLanguage: English - Date: 2012-08-14 14:53:32
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4![A Variability Survey of Bright Stars on the Ecliptic Plane with STEREO K.T. Wraight¹, G.J. White¹ ², D. Bewsher³, A.J. Norton¹ Comparison of STEREO characteristics (1) Department of Physics and Astronomy, The Open A Variability Survey of Bright Stars on the Ecliptic Plane with STEREO K.T. Wraight¹, G.J. White¹ ², D. Bewsher³, A.J. Norton¹ Comparison of STEREO characteristics (1) Department of Physics and Astronomy, The Open](https://www.pdfsearch.io/img/0d8a1377c4d7a7b509da21c03120eeba.jpg) | Add to Reading ListSource URL: www.star.uclan.ac.ukLanguage: English - Date: 2011-04-11 13:22:00
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5![K2 Campaign 2&3 Proposal for Monitoring Cataclysmic Variables Paula Szkody & Zhibin Dai (U of Washington); Peter Garnavich (U of Notre Dame) The original Kepler field had 27 cataclysmic variables (CVs:close binaries with K2 Campaign 2&3 Proposal for Monitoring Cataclysmic Variables Paula Szkody & Zhibin Dai (U of Washington); Peter Garnavich (U of Notre Dame) The original Kepler field had 27 cataclysmic variables (CVs:close binaries with](https://www.pdfsearch.io/img/a79ed6b35955f258c1c0cba9f0577f6a.jpg) | Add to Reading ListSource URL: keplerscience.arc.nasa.govLanguage: English - Date: 2015-04-02 16:37:17
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6![Long cadence observations of cataclysmic variables with K2 S. Scaringi1,2 , P. Groot3 , C. Knigge4 , E. Koerding3 , K.S. Long5 , T. Maccarone6 1 K.U. Leuven, Leuven, Belgium, 2 Max Planck Institute for Extraterrestrial P Long cadence observations of cataclysmic variables with K2 S. Scaringi1,2 , P. Groot3 , C. Knigge4 , E. Koerding3 , K.S. Long5 , T. Maccarone6 1 K.U. Leuven, Leuven, Belgium, 2 Max Planck Institute for Extraterrestrial P](https://www.pdfsearch.io/img/38543547effe8b32964e50f758f09077.jpg) | Add to Reading ListSource URL: keplerscience.arc.nasa.govLanguage: English - Date: 2015-04-02 16:37:17
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7![Cataclysmic variables can be defined as stars that have periods of inactivity interrupted by changes in brightness Cataclysmic variables can be defined as stars that have periods of inactivity interrupted by changes in brightness](https://www.pdfsearch.io/img/8b3f341cb6bc0b340f2bdc877c5d3a07.jpg) | Add to Reading ListSource URL: phys.udallas.eduLanguage: English - Date: 2006-10-17 17:05:12
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8![PRESS RELEASE Released on 5 November 2009 German high-school students involved in an astronomical research project on cataclysmic variable stars PRESS RELEASE Released on 5 November 2009 German high-school students involved in an astronomical research project on cataclysmic variable stars](https://www.pdfsearch.io/img/761b105e65ee0412ee1c8b95fda46800.jpg) | Add to Reading ListSource URL: www.aanda.orgLanguage: English - Date: 2015-03-31 04:48:30
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9![HPOL: World’s Largest Database of Optical Spectropolarimetry M.R. Meade, B.L. Babler, B.A. Whitney, K.H. Nordsieck, K.S. Bjorkman, J.P. Wisniewski, A.M. Magalhaes, M.J. Wolff Stars with a V magnitude range of 0.1 to 12 HPOL: World’s Largest Database of Optical Spectropolarimetry M.R. Meade, B.L. Babler, B.A. Whitney, K.H. Nordsieck, K.S. Bjorkman, J.P. Wisniewski, A.M. Magalhaes, M.J. Wolff Stars with a V magnitude range of 0.1 to 12](https://www.pdfsearch.io/img/c030ad8fa78bda2bbd025f81c59a5f37.jpg) | Add to Reading ListSource URL: www.sal.wisc.eduLanguage: English - Date: 2011-08-10 16:44:10
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10![Kepler K2 observations of the bright intermediate polar FO Aquarii C OEL H ELLIER , K EELE U NIVERSITY Accretion disks are widespread in astrophysics, from the formation of stars and planets to the brightest AGN. Catacly Kepler K2 observations of the bright intermediate polar FO Aquarii C OEL H ELLIER , K EELE U NIVERSITY Accretion disks are widespread in astrophysics, from the formation of stars and planets to the brightest AGN. Catacly](https://www.pdfsearch.io/img/698f39f8fe41fc893f29337c6cbda426.jpg) | Add to Reading ListSource URL: keplerscience.arc.nasa.govLanguage: English - Date: 2014-12-01 19:16:20
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