HS0907+1902 = GY Cnc = RX J0909.8+1849

A deeply eclipsing 4h orbital period dwarf nova with relatively infrequeny outbursts. Very nice object, but does not really need additional attention as it is already well-monitored.

Literature

Jiang, X. J., Engels, D., Wei, J. Y., Tesch, F., Hu, J. Y., 2000. New cataclysmic variables from the RASS, Astronomy & Astrophysics 362, 263

Gänsicke, B. T., Fried, R. E., Hagen, H.-J., Beuermann, K., Engels, D., Hessman, F. V., Nogami, D., Reinsch, K. 2000. HS 0907+1902: a new 4.2 hr eclipsing dwarf nova, Astronomy & Astrophysics 356L, 79

Shafter, A. W., Clark, L. Lee, Holland, Julia, Williams, Stephen J., 2000. A Time-resolved Photometric Study of the Eclipsing Dwarf Nova RX J0909+1849, PASP 112, 1467

Thorstensen, J.R., 2000. Spectroscopy and Component Masses of the Eclipsing Dwarf Nova HS 0907+1902, PAPS 112, 1269

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