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UBV photometry of HD stars in the fields of selected cataclysmic variables.
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| Multiwavelength monitoring of the dwarf nova VW Hydri. II - Walraven photometry
Five-color Walraven photometric observations of VW Hyi were obtainedbetween July and November 1984. Significant orbital variations in theV-B, B-U, and B-L colors are detected which are mainly connected withthe presence of an orbital hump. No evidence is found for a secularvariation between outbursts in either the average flux or the orbitalmaximum and minimum fluxes, and little evidence is found for a seculartrend in the shape of the orbital light curves between outbursts. Theflux ratio across the Balmer jump is shown to change during a quiescenceinterval between outbursts, and results suggest a secular change in theshape of the B-U and U-W orbital color curves through quiescence. Theonset of normal outbursts is found to be progressively delayed towardsshorter wavelengths, in agreement with IUE observations.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Hydrus |
| Ascensió Recta: | 04h10m20.15s |
| Declinació: | -71°20'38.6" |
| Magnitud Aparent: | 9.409 |
| Moviment propi RA: | -45.4 |
| Moviment propi Dec: | -103.6 |
| B-T magnitude: | 10.266 |
| V-T magnitude: | 9.48 |
Catàlegs i designacions:
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