| dc.contributor.author | Selam, SO | |
| dc.contributor.author | Ak, T | |
| dc.contributor.author | Elmasli, A | |
| dc.contributor.author | Ozavci, I | |
| dc.contributor.author | Albayrak, B | |
| dc.date.accessioned | 2021-03-05T08:06:40Z | |
| dc.date.available | 2021-03-05T08:06:40Z | |
| dc.date.issued | 2005 | |
| dc.identifier.citation | Albayrak B., Selam S., Ak T., Elmasli A., Ozavci I., "Light-time effect in the eclipsing binary system AM Leonis", ASTRONOMISCHE NACHRICHTEN, cilt.326, ss.122-126, 2005 | |
| dc.identifier.issn | 0004-6337 | |
| dc.identifier.other | av_97352875-fec1-4892-a157-f2cc02a7b62d | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/101788 | |
| dc.identifier.uri | https://doi.org/10.1002/asna.200410349 | |
| dc.description.abstract | We report four new times of minimum light and the improved ephemeris for the well known contact binary AM Leo. The O-C diagram, constructed with all reliable timings found in the literature was analyzed and the the light-time effect in the system was confirmed. We found a periodicity of 44.82 years in the O-C residuals with an amplitude of 0.0058 day. The periodic curve representing the O-C values is asymmetric indicating a large eccentricity of 0.73 of the third body orbit. The mass of the third body is found to be 0.175 M-circle dot for the orbital inclination of the eclipsing pair's orbit. | |
| dc.language.iso | eng | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.subject | Uzay bilimi | |
| dc.subject | Fizik | |
| dc.subject | Temel Bilimler | |
| dc.title | Light-time effect in the eclipsing binary system AM Leonis | |
| dc.type | Makale | |
| dc.relation.journal | ASTRONOMISCHE NACHRICHTEN | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 326 | |
| dc.identifier.issue | 2 | |
| dc.identifier.startpage | 122 | |
| dc.identifier.endpage | 126 | |
| dc.contributor.firstauthorID | 53913 | |
