dc.contributor.author |
Abhyankar, K. D |
|
dc.contributor.author |
Panchatsaram, T |
|
dc.date.accessioned |
2005-02-09T06:11:31Z |
|
dc.date.available |
2005-02-09T06:11:31Z |
|
dc.date.issued |
1982-12 |
|
dc.identifier.citation |
BASI, Vol. 10, No. 4, pp. 315-322 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/349 |
|
dc.description.abstract |
An analysis of the minimum-time data of AK Her and ER Ori revelas possible sinudodal variations in their orbital periods. In the case of AK Her we suspect two additional components; one of mass 0.2 to 0.4 MSun with a period of 62 yr and the other of mass 0.2 to 0.6 MSun with a period of 207 yr. The probable third mass in ER Ori is less than 0.6 MSun for i>or equal to 60 degree with a long-term period of 34.78 yr. |
en |
dc.format.extent |
586715 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
|
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
AK Her |
en |
dc.subject |
ER Ori |
en |
dc.subject |
minimum-time data |
en |
dc.title |
Light-time effect in AK Her and ER Ori |
en |
dc.type |
Article |
en |