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Norton, A. J.; Quaintrell, H.; Katajainen, S.; Lehto, H. J.; Mukai, K. and Negueruela, I.
(2002).
DOI: https://doi.org/10.1051/0004-6361:20011820
Abstract
We present optical photometry, spectroscopy and photopolarimetry, as well as ASCA X-ray observations, of the recently discovered intermediate polar 1WGA J1958.2+3232. Through the first detection of an optical beat frequency, we confirm the previously tentative suggestion that the spin period of the white dwarf is twice the X-ray and optical pulsation period, which we also confirm in each case. We detect an orbital modulation in each of the U, B, V, R and I bands for the first time, and suggest that the true orbital period is the -1d alias of that previously suggested. We also confirm the presence of circular polarization in this system, detecting a variable polarization which has opposite signs in each of the B and R bands. The double peaked pulse profile and oppositely signed polarization pulses suggest that 1WGA J1958.2+3232 accretes onto both magnetic poles via a disc which is truncated relatively close to the white dwarf.
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About
- Item ORO ID
- 4423
- Item Type
- Journal Item
- ISSN
- 1432-0746
- Project Funding Details
-
Funded Project Name Project ID Funding Body Not Set PPA/G/O/2000/00037 PPARC Not Set GR/L64621 PPARC Not Set 71355 Finnish Academy Not Set 44011 Finnish Academy - Keywords
- novae; cataclysmic variables; stellar magnetic fields; 1WGA J1958.2+3232
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2002 ESO
- Depositing User
- Users 6827 not found.