共 41 条
CoRoT-TESS eclipsing binaries with light-travel-time effect
被引:5
作者:
Hajdu, T.
[1
,2
,3
,4
]
Matecsa, B.
[3
]
Sallai, J. M.
[3
]
Bodi, A.
[1
,2
,4
]
机构:
[1] Konkoly Observ Res Ctr Astron & Earth Sci ELKH, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary
[2] MTA Ctr Excellence, CSFK, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary
[3] Eotvos Lorand Univ, Dept Astron, Pazmany Peter Stny 1-A, H-1118 Budapest, Hungary
[4] MTA CSFK Lendulet Near Field Cosmol Res Grp, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary
关键词:
methods: numerical;
binaries: close;
binaries: eclipsing;
HIERARCHICAL TRIPLE SYSTEM;
ORBITAL PERIOD MODULATION;
TIMING VARIATION ANALYSIS;
GALACTIC BULGE;
LONGITUDES;
MECHANISM;
YOUNG;
1ST;
I;
D O I:
10.1093/mnras/stac2533
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Identifying long-period eclipsing binaries with space-based photometry is still a challenge even in the century of space telescopes due to the relatively short observation sequences and short lifetime of these missions. The Transiting Exoplanet Survey Satellite (TESS) space telescope is an appropriate tool to supplement previous space-based observations. In this paper, we report the first results of the eclipse timing variation (ETV) analyses of eclipsing binaries (EBs) measured by CoRoT and TESS space telescopes. Among the 1428 EB candidates we found four new potential triple candidates, for which ETV was analysed and fitted by the well-known light-travel-time effect (LTTE). One of them shows significant phase shift in its folded light curve which required extra care. In this paper, we also present some other systems showing significant ETV signals that could be explained by mass transfer or apsidal motion.
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页码:5165 / 5170
页数:6
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