dc.contributor.author | Panchatsaram, T | |
dc.date.accessioned | 2005-02-04T16:14:44Z | |
dc.date.available | 2005-02-04T16:14:44Z | |
dc.date.issued | 1981-06 | |
dc.identifier.citation | BASI, Vol. 9, No. 2, pp. 139-143 | en |
dc.identifier.uri | http://hdl.handle.net/2248/311 | |
dc.description.abstract | With the available photoelectric times of minima the variations in the orbital period of U Oph can be interpreted in terms of the presence of a third body. | en |
dc.format.extent | 327355 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en | |
dc.publisher | Astronomical Society of India | en |
dc.subject | eclipsing binaries | en |
dc.subject | period changes | en |
dc.subject | light time effect | en |
dc.title | A study of the period of U Ophiuchi | en |
dc.type | Article | en |