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| UBV photometry of HD stars in the fields of selected cataclysmic variables. Not Available
| Photometry and polarimetry of VW Hydri during the October 1978 supermaximum The photoelectric observations of VW Hyi at the supermaximum show thesuperhump phenomenon which weakens during the decline, with severalpeaks appearing in the light curve. One peak developed near phase 0.5P(1) for several days, and interfered with the orbital hump producingthe beat phenomenon; two ultrashort period oscillations of 33 and 74 soccurred near the detection limit. The nightly mean linear polarizationwas in the 0.02-0.1% range, increasing with decreasing brightness; thepolarization was caused by a single particle scattering in the disk. Thecolor curves suggest that the disk has a more spherical shape in theearly outbursts state than during quiescence, and it gradually flattensduring the decline.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
Constel·lació: | Hydrus |
Ascensió Recta: | 04h08m33.52s |
Declinació: | -71°38'23.5" |
Magnitud Aparent: | 8.656 |
Distancia: | 96.339 parsecs |
Moviment propi RA: | 38.3 |
Moviment propi Dec: | 105.5 |
B-T magnitude: | 9.19 |
V-T magnitude: | 8.701 |
Catàlegs i designacions:
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