IGR J17303-0601 is a new intermediate polar

Gaensicke, B. T.; Marsh, T. R.; Edge, A.; Rodriguez-Gil, P.; Steeghs, D.; Araujo-Betancor, S.; Harlaftis, E.; Giannakis, O.; Pyrzas, S.; Morales-Rueda, L.; Aungwerojwit, A.
Referencia bibliográfica

The Astronomer's Telegram, #463

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4
2005
Número de autores
11
Número de autores del IAC
0
Número de citas
5
Número de citas referidas
5
Descripción
We have identified IGR J17303-0601 (1RXS J173021.5-055933) as an intermediate polar (IP). The optical counterpart is USNOA2.0 0825_10606993 (RA=17h30m21.9s Dec=-05d59m31s). Using optical photometry obtained in 2003 at the JKT and at the OGS we determine the white dwarf spin period to be 120s, which is the second-shortest spin period discovered so far (after AE Aqr, Pspin=33s). The spin folded light curve has a double-pulse structure, suggesting that both accreting poles / accretion curtains contribute to the optical light.