Photometric Study on the Spot-Double Star XY Ursae Majoris (II)
The photometric behaviour of XY UMa, an eclipsing binary showing photospheric and chromospheric activity, has been described by spot hypothesis. They are based on the all the available UBV light curves, which were carried out by Geyer since 1955. A "spherical rectangular" spot model shows very prono...
Сохранить в:
| Главный автор: | |
|---|---|
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
The Korean Space Science Society
1988-12-01
|
| Серии: | Journal of Astronomy and Space Sciences |
| Online-ссылка: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_97.pdf |
| Метки: |
Нет меток, Требуется 1-ая метка записи!
|
