Abstract
A significant number of close binaries are known to be members of physically bound triple or multiple star systems. The O - C analysis technique which is based on the minima times of an eclipsing binary can reveal the light-time effect due to the presence of gravitationally bound and generally unseen close component(s) in the system. In this study we present shortly the O - C analysis results based on the light-time effect possibilities for two of the eclipsing binaries observationally followed by our group; TZ Boo and CF Tau.
Original language | English |
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Pages (from-to) | 131-133 |
Number of pages | 3 |
Journal | Astrophysics and Space Science |
Volume | 304 |
Issue number | 1-4 |
DOIs | |
Publication status | Published - Aug 2006 |
Externally published | Yes |
Keywords
- Binaries: close
- Binaries: eclipsing
- TZ Boo and CF Tau