The multiple nature of CC Com: One of the ultra-short orbital period late-type contact binary systems
Küçük Resim Yok
Tarih
2024
Yazarlar
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Cambridge University Press
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
The study of very short-period contact binaries provides an important laboratory in which the most important and problematic astrophysical processes of stellar evolution take place. Short-period contact systems, such as CC Com, are particularly important for binary evolution. Close binary systems, especially those with multiple system members, have significant period variations, angular momentum loss mechanisms predominance, and pre-merger stellar evolution, making them valuable astrophysical laboratories. In this study, observations of CC Com, previously reported as a binary system, and new observations from the T & Uuml;B & Idot;TAK National Observatory (TUG) and the space-based telescope TESS have revealed that there is a third object with a period of about eight years and a fourth object with a period of about a century orbiting the binary system. From simultaneous analysis of all available light curves and radial velocities, the sensitive orbital and physical parameters of the system components are derived. The orbital parameters of the components are PA=0.2206868 +/- 0.0000002 days,P-B=7.9 +/- 0.1 yr, P-C=98 +/- 5yr,e3=0.06,e4=0.44 and the physical parameters as M-A1=0.712 +/- 0.009 M-circle dot,M-A2=0.372 +/- 0.005 M-circle dot,m(B;i ')=90 degrees=0.074 M-circle dot,m(C;i ')=90 degrees=0.18 M-circle dot,R-A1=0.693 +/- 0.006 R-circle dot,R-A2=0.514 +/- 0.005 R-circle dot,L-A1=0.103 L-circle dot,L-A2=0.081 L-circle dot. Finally, theevolutionary status of the multiple system CC Com and its component stars is discussed
Açıklama
Anahtar Kelimeler
(stars:) Binaries (including multiple): close, methods: observational, stars: evolution, techniques: photometric, techniques: radial velocities
Kaynak
Publications of the Astronomical Society of Australia
WoS Q Değeri
Q1
Scopus Q Değeri
Q1
Cilt
41
Sayı
Sep
Künye
Kocak, D. (2024). The multiple nature of CC com: One of the ultra-short orbital period late-type contact binary systems. Publications of the Astronomical Society of Australia, 41
