A Period Study of the Close Binary V651 Cassiopeiae
All times of minimum light of V651 Cas, which is still less studied so far, were analyzed. From our analysis, it was found that the orbital period of the system may have varied in a periodic manner. After assuming that the period change is produced by the light-time effect due to a third body in the...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
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The Korean Space Science Society
2000-12-01
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| Series: | Journal of Astronomy and Space Sciences |
| Subjects: | |
| Online Access: | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n2/OJOOBS_2000_v17n2_173.pdf |
| _version_ | 1797370443119722496 |
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| author | Chun-Hwey Kim Jae Woo Lee |
| author_facet | Chun-Hwey Kim Jae Woo Lee |
| author_sort | Chun-Hwey Kim |
| collection | DOAJ |
| description | All times of minimum light of V651 Cas, which is still less studied so far, were analyzed. From our analysis, it was found that the orbital period of the system may have varied in a periodic manner. After assuming that the period change is produced by the light-time effect due to a third body in the system, attempts to derive the orbital elements of the light-time orbit were made. The resultant values for the period, semi-amplitude, and eccentricity of the light-time orbit were 6.y25, 0.d0013, and 0.77, respectively. The future observations of times of minimum light of V651 Cas are needed to confirm the existence of the third body we suggested in this paper. |
| first_indexed | 2024-03-08T18:02:40Z |
| format | Article |
| id | doaj.art-a9880b8c4b874d09ba2a91b54922687e |
| institution | Directory Open Access Journal |
| issn | 2093-5587 2093-1409 |
| language | English |
| last_indexed | 2024-03-08T18:02:40Z |
| publishDate | 2000-12-01 |
| publisher | The Korean Space Science Society |
| record_format | Article |
| series | Journal of Astronomy and Space Sciences |
| spelling | doaj.art-a9880b8c4b874d09ba2a91b54922687e2024-01-02T00:32:57ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092000-12-01172173180A Period Study of the Close Binary V651 CassiopeiaeChun-Hwey Kim0Jae Woo Lee1Department of Astronomy and Space Science, Chungbuk National UniversityKorea Astronomy Observatory All times of minimum light of V651 Cas, which is still less studied so far, were analyzed. From our analysis, it was found that the orbital period of the system may have varied in a periodic manner. After assuming that the period change is produced by the light-time effect due to a third body in the system, attempts to derive the orbital elements of the light-time orbit were made. The resultant values for the period, semi-amplitude, and eccentricity of the light-time orbit were 6.y25, 0.d0013, and 0.77, respectively. The future observations of times of minimum light of V651 Cas are needed to confirm the existence of the third body we suggested in this paper.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n2/OJOOBS_2000_v17n2_173.pdfSTARSCLOSE BINARIESPERIOD VARIATION |
| spellingShingle | Chun-Hwey Kim Jae Woo Lee A Period Study of the Close Binary V651 Cassiopeiae Journal of Astronomy and Space Sciences STARS CLOSE BINARIES PERIOD VARIATION |
| title | A Period Study of the Close Binary V651 Cassiopeiae |
| title_full | A Period Study of the Close Binary V651 Cassiopeiae |
| title_fullStr | A Period Study of the Close Binary V651 Cassiopeiae |
| title_full_unstemmed | A Period Study of the Close Binary V651 Cassiopeiae |
| title_short | A Period Study of the Close Binary V651 Cassiopeiae |
| title_sort | period study of the close binary v651 cassiopeiae |
| topic | STARS CLOSE BINARIES PERIOD VARIATION |
| url | http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2000/v17n2/OJOOBS_2000_v17n2_173.pdf |
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