Norton, A.J.; Quaintrell, H. and Negueruela, I.
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UBV RI observations of the recently identified intermediate polar 1WGA J1958.2+3232 reveal that the pulsation period of 733 s is half the white dwarf spin period and demonstrate the existence of an optical beat modulation. An orbital modulation is detected in all wavebands, but the previously identified orbital period is likely to be an alias.
|Item Type:||Conference Item|
|Copyright Holders:||2002 Astronomical Society of the Pacific|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 6827 not found.|
|Date Deposited:||07 Jul 2006|
|Last Modified:||02 Aug 2016 12:58|
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