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Issue A&A
Volume 390, Number 3, August II 2002
Page(s) L23 - L26
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:20020913



A&A 390, L23-L26 (2002)
DOI: 10.1051/0004-6361:20020913

Letter

On the orbital period of the Intermediate Polar 1WGA J1958.2+3232

S. V. Zharikov1, G. H. Tovmassian1 and J. Echevarría2

1  Observatorio Astronómico Nacional, Instituto de Astronomía, UNAM, 22800, Ensenada, B.C., México (Use for smail PO Box 439027, San Diego, CA, 92143-9027, USA.)
2  Instituto de Astronomía, UNAM, Apartado Postal 70-264, 04510 México, D.F., México

(Received 11 April 2002 / Accepted 17 June 2002)

Abstract
Recently, Norton et al. (2002), on the basis of multiwavelength photometry of 1 WGA J1958.2+3232, argued that the -1 day alias of the strongest peak in the power spectrum is the true orbital period of the system, casting doubts on the period estimated by Zharikov et al. (2001). We re-analyzed this system using our photometric and spectroscopic data along with the data kindly provided by Andy Norton and confirm our previous finding. After refining our analysis we find that the true orbital period of this binary system is 4 $\fh$35.


Key words: stars: individual: 1 WGA J1958.2+3232 -- stars: novae, cataclysmic variables -- stars: binaries: close -- X-rays

Offprint request: S. V. Zharikov, zhar@astrosen.unam.mx

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