Emilios Theofanus Harlaftis

Affiliations: 
2002-2005 National Observatory of Athens 
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https://en.wikipedia.org/wiki/Emilios_T._Harlaftis
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"Emilios Theofanus Harlaftis"
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Cross-listing: Physics Tree

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Phil A. Charles grad student 1991 Oxford (Physics Tree)
 (Disc structure and variability in dwarf novae.)
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Van Oers P, Markoff S, Rahoui F, et al. (2010) Is the plateau state in GRS 1915+105 equivalent to canonical hard states? Monthly Notices of the Royal Astronomical Society. 409: 763-776
Martin AC, Charles PA, Callanan PJ, et al. (2008) The periodicities of AQL X‐1 in quiescence The Evolution of X‐Ray Binaries. 308: 127-130
Harlaftis E, Jones D, Charles P, et al. (2008) ING photometry and spectroscopy of the optical counterpart of the x‐ray transient GRO J0422+32 The Evolution of X‐Ray Binaries. 308: 91-94
Dhillon VS, Marsh TR, Stevenson MJ, et al. (2007) ULTRACAM: An ultrafast, triple-beam CCD camera for high-speed astrophysics Monthly Notices of the Royal Astronomical Society. 378: 825-840
Rodriguez-Gil P, Gansicke BT, Hagen HJ, et al. (2007) SW Sextantis stars: the dominant population of cataclysmic variables with orbital periods between 3 and 4 h Monthly Notices of the Royal Astronomical Society. 377: 1747-1762
Ribeiro T, Baptista R, Harlaftis ET, et al. (2007) A multicolor near-infrared study of the dwarf nova IP Pegasi Astronomy and Astrophysics. 474: 213-220
Hernández JIG, Rebolo R, Israelian G, et al. (2006) XTE J1118+480: A Metal-rich Black Hole Binary in the Galactic Halo The Astrophysical Journal. 644
Aungwerojwit A, Gänsicke BT, Rodríguez-Gil P, et al. (2006) Dwarf novae in the Hamburg quasar survey: rarer than expected Astronomy and Astrophysics. 455: 659-672
Giannakis O, Harlaftis ET, Niarchos PG, et al. (2006) Mapping of the Disc Structure of the Neutron Star X-ray Binary X1822-371 Astrophysics and Space Science. 304: 321-322
Papadimitriou C, Harlaftis E, Steeghs D. (2006) The Structure and the Partial Opacity of the Spiral Shocks on the Novalike Cataclysmic Variables Astrophysics and Space Science. 304: 315-316
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