Monitoring of the Cataclysmic Variable TW Tri

Details Monitoring of the Cataclysmic Variable TW Tri Monitoring of the Cataclysmic Variable TW Tri

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..424..216p&link_type=abstract

Proceedings of the 9th International Conference of the Hellenic Astronomical Society, proceedings of a conference held 20-24 Sep

Astronomy and Astrophysics

Astronomy

Scientific paper

We present white light CCD photometry and Fourier power spectrum analysis of the dwarf nova TW Trianguli (TW Tri). Data have been collected from eight different epochs between September 2006 and September 2008, using the 1.2 m Kryoneri telescope of the National Observatory of Athens in Greece. We find, for the first time using photometric data, that the orbital period of the system is Porb ˜ 0.21 days.

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