1996PASP..108..130S

Query : 1996PASP..108..130S

1996PASP..108..130S - Publ. Astron. Soc. Pac., 108, 130-133 (1996/February-0)

Photometry of the new DQ Her star RX J0558.0+5353.

SKILLMAN D.R.

Abstract (from CDS):

Times series CCD photometry of RX J0558.0+5353 reveals optical variations similar to the X-ray variations seen by ROSAT. These variations are about 0.04 magnitudes (semiamplitude) in unfiltered light. Fourier analysis of these time series indicates that the rotation period of the white dwarf is twice the reported X-ray period. The WD rotation period determined by pulse timings over a 138 baseline is 545.4565(8) seconds. Detailed examination of pulse arrival times shows a small variation in arrival time depending on orbital phase.

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Journal keyword(s): Stars

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* V405 Aur CV* 05 57 59.2934496792 +53 53 44.926489464           ~ 140 0
2 V* DO Dra CV* 11 43 38.4921265896 +71 41 20.559036192       13.747   DQ 233 1
3 V* DQ Her CV* 18 07 30.2510391864 +45 51 32.564791872   14.605 14.443 14.800   M3+Ve 1048 1
4 V* AE Aqr CV* 20 40 09.1598959176 -00 52 15.055595220   12.46 10.40   10.191 K3-5IV/V 705 0

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