A cyclical period variation detected in the updated orbital period analysis of TV Columbae
Two CCD photometries of the intermediate polar TV Columbae are made for obtaining two updated eclipse timings with high precision. There is an interval time ~17 yr since the last mid-eclipse time observed in 1991. Thus, the new mid-eclipse times might offer an opportunity to check the previous orbit...
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| Autores principales: | , , , |
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| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2010
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93867 https://link.springer.com/article/10.1007%2Fs10509-010-0412-0 |
| Aporte de: |
| id |
I19-R120-10915-93867 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Astronomía Cataclysmic variables Eclipsing binaries TV Columbae (estrella) |
| spellingShingle |
Astronomía Cataclysmic variables Eclipsing binaries TV Columbae (estrella) Dai, Zhibin Qian, Shengbang Fernández Lajús, Eduardo Eusebio Baume, Gustavo Luis A cyclical period variation detected in the updated orbital period analysis of TV Columbae |
| topic_facet |
Astronomía Cataclysmic variables Eclipsing binaries TV Columbae (estrella) |
| description |
Two CCD photometries of the intermediate polar TV Columbae are made for obtaining two updated eclipse timings with high precision. There is an interval time ~17 yr since the last mid-eclipse time observed in 1991. Thus, the new mid-eclipse times might offer an opportunity to check the previous orbital ephemerides. A calculation indicates that the orbital ephemeris derived by Augusteijn et al. (Astron. Astrophys. Suppl. Ser. 107:219, 1994) should be corrected. Based on the proper linear ephemeris (Hellier in Mon. Not. R. Astron. Soc. 264:132, 1993), the new orbital period analysis suggests a cyclical period variation in the O-C diagram of TV Columbae. Using Applegate's mechanism to explain the periodic oscillation in the O-C diagram, the required energy is larger than the energy that a M0-type star can afford over a complete variation period of ~31.0(±3.0) yr. Thus, the light travel-time effect indicates that the tertiary component in TV Columbae may be a dwarf with a low mass, which is near the lower mass limit of ~0.08M⊙ as long as the inclination of the third body is high enough. |
| format |
Articulo Preprint |
| author |
Dai, Zhibin Qian, Shengbang Fernández Lajús, Eduardo Eusebio Baume, Gustavo Luis |
| author_facet |
Dai, Zhibin Qian, Shengbang Fernández Lajús, Eduardo Eusebio Baume, Gustavo Luis |
| author_sort |
Dai, Zhibin |
| title |
A cyclical period variation detected in the updated orbital period analysis of TV Columbae |
| title_short |
A cyclical period variation detected in the updated orbital period analysis of TV Columbae |
| title_full |
A cyclical period variation detected in the updated orbital period analysis of TV Columbae |
| title_fullStr |
A cyclical period variation detected in the updated orbital period analysis of TV Columbae |
| title_full_unstemmed |
A cyclical period variation detected in the updated orbital period analysis of TV Columbae |
| title_sort |
cyclical period variation detected in the updated orbital period analysis of tv columbae |
| publishDate |
2010 |
| url |
http://sedici.unlp.edu.ar/handle/10915/93867 https://link.springer.com/article/10.1007%2Fs10509-010-0412-0 |
| work_keys_str_mv |
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Repositorios |
| _version_ |
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