Astrometric solution of the multiple system XY Leo
[ X ]
Tarih
2005
Yazarlar
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Springer
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
An astrometric solution, together with time of minimum analysis, has been made for the multiple system XY Leonis (HIP 49136) to identify the properties of the remote companion to the eclipsing pair (AB). From this solution, we derive the inclination of the wide orbit (AB-cd) as 94.4 degrees +/- 0.2 degrees, angle of nodes as 247.3 degrees +/- 0.2 degrees, and the mass of the wide component (the dwarf binary cd) as 0.98 +/- 0.2 M-.. This study confirms that the light travel time effect can explain the sinusoidal O - C variation of the eclipsing system.
Açıklama
International Conference on Zdenek Kopals Binary Star Legacy -- MAR 31-APR 03, 2004 -- Litomysl, CZECH REPUBLIC
Anahtar Kelimeler
eclipsing binaries, triple systems, astrometry, light time effect
Kaynak
Astrophysics and Space Science
WoS Q Değeri
Q4
Scopus Q Değeri
Q2
Cilt
296
Sayı
1-4
