Ýçindekiler
Görüntüler
Resim Yükleyin
DSS Images Other Images
Ýlgili Makaleler
Apsidal Motion and Photometric Elements of the Eccentric Eclipsing Binary V401 Lacertae
New (UBV) photometric observations of the recently discovered eccentricorbit binary V401 Lacertae were analyzed by using the Wilson-Devinneyprogram. Seven new minimum times were estimated by using newobservations. The analysis of the light curves and all available minimumtimes has revealed that the system is detached, with the orbitaleccentricity e = 0.1734 ± 0.0003, the longitude of the periastronω = 63.°93 ± 0.°15, the rate of change of thelongitude of periastron dot{ω} = 0.°0200 ± 0.°0024cycle-1, corresponding to an apsidal motion period of U =96.2 ± 11.4 yr. The apsidal motion of the system has beenconfirmed by the significant difference on the longitude of periastron(ω) obtained from two light curves (Hipparcos and ourselves) intwo different epochs.
|
Yeni bir Makale Öner
Ýlgili Baðlantýlar
Yeni Bir Baðlantý Öner
sonraki gruplarýn üyesi:
|
Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Kertenkele |
| Sað Açýklýk: | 22h05m13.07s |
| Yükselim: | +49°18'45.5" |
| Görünürdeki Parlaklýk: | 8.247 |
| Uzaklýk: | 254.453 parsek |
| özdevim Sað Açýklýk: | 0.2 |
| özdevim Yükselim: | -14.9 |
| B-T magnitude: | 8.409 |
| V-T magnitude: | 8.261 |
Kataloglar ve belirtme:
|
