dc.contributor.author |
Srivastava, R. K. |
|
dc.date.accessioned |
2010-02-18T06:07:42Z |
|
dc.date.available |
2010-02-18T06:07:42Z |
|
dc.date.issued |
1987 |
|
dc.identifier.citation |
This article is downloaded for ADS |
en_US |
dc.identifier.uri |
http://hdl.handle.net/123456789/545 |
|
dc.description.abstract |
A first period study of the eclipsing RS CVn-binary RW Com is presented. A new period (p=0.ͩ 2373455) based on 223 minima is given. The O-C diagrams of RW Com have been presented for the first time. Types of ten minima have been corrected judging the period trend. Period changes in different portions of the O-C diagram (Figure 2) have been estimated. The total change in period (ΔP/P) ranges from 5.5x10⁻⁷ to 6.4x10⁻⁶. Thus, ΔP ranges from 1.3x10⁻⁷d to 1.5x10⁻⁶d. Numerous minima are available in the time interval 1967 to 1986. This part of the O-C diagram (Figure 2) shows a sinusoidal variation, thus, it is suspected that RW Com could be a three-body system. The period of variation due to third body appears to be nearly 16 years. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
ass139-373 |
|
dc.subject |
RS CVn-binary RW Com system |
en_US |
dc.title |
RS CVn-binary RW Com: a possible three-body system |
en_US |
dc.type |
Article |
en_US |