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Intensive photometry of southern Wolf-Rayet stars Results of an intensive photometric campaign on 17 of the brightestsouthern Wolf-Rayet stars are presented. The detection ofmultiperiodicity in two stars, HD 50896 and HD 96548, is reported. It islikely that these periodicities are not coherent but are manifestationsof the quasi-periodic variations seen in a few WR stars. A good exampleof these variations is given by HD 86161. A new eclipsing binary, HD92740, has been discovered; other stars show periodic variations whichcan be explained by phase-dependent scattering of the secondary light asit traverses the Wolf-Rayet wind. An important conclusion of this studyis that not a single example was found of short-period variations whichcan be attributed to pulsation.
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Gözlemler ve gökölçümü verileri
Takýmyýldýz: | Guney Ucgeni |
Sað Açýklýk: | 16h06m27.39s |
Yükselim: | -63°20'28.2" |
Görünürdeki Parlaklýk: | 7.549 |
Uzaklýk: | 150.83 parsek |
özdevim Sað Açýklýk: | -29.3 |
özdevim Yükselim: | -26.8 |
B-T magnitude: | 7.655 |
V-T magnitude: | 7.558 |
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