1998 UBV observations of ST Aquarii and light curve analysis

Citation
Dmz. Jassur et al., 1998 UBV observations of ST Aquarii and light curve analysis, ASTRO SP SC, 272(4), 2000, pp. 319-324
Citations number
11
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICS AND SPACE SCIENCE
ISSN journal
0004640X → ACNP
Volume
272
Issue
4
Year of publication
2000
Pages
319 - 324
Database
ISI
SICI code
0004-640X(2000)272:4<319:1UOOSA>2.0.ZU;2-L
Abstract
1998 UBV photometry of short period eclipsing binary ST Aquarii have been p resented. The photometric solution obtained from light curve analysis by th e method of differential corrections indicates that the system can be class ified as a near contact binary. Derived value for the ratio of radii (k = [ r(h)]/[r(c)] congruent to 0.67) shows that both components cannot be consid ered to be Main-Sequence, but they are probably evolved from M.S.