Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6179
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dc.contributor.authorSanwal, N. B-
dc.contributor.authorSarma, M. B. K-
dc.contributor.authorVivekanand Rao, P-
dc.contributor.authorParthasarathy, M-
dc.date.accessioned2013-07-10T13:45:55Z-
dc.date.available2013-07-10T13:45:55Z-
dc.date.issued1990-03-
dc.identifier.citationContributions from the Nizamiah and Japal-Rangapur Observatories, Hyderabad, India. Contribution No. 24, March 1990, pp. 1-30en
dc.identifier.urihttp://hdl.handle.net/2248/6179-
dc.descriptionOpen Accessen
dc.description.abstractThe short-period eclipsing binary V Crateris is observed in the B and V colors of Johnson and Morgan's UBV system with attention given to the results from comparison and check stars. Magnitude differences are listed, and the standard observational error is given at 0.010 mag both for V and B filters. Observational data for V Crateris are given with the heliocentric Julian day and the magnitude difference in the standard system.en
dc.language.isoenen
dc.publisherOsmania Universityen
dc.relation.ispartofseriesNizamiah and Japal-Rangapur Observatories Hyderabad, India, Contribution;24-
dc.rights©Osmania Universityen
dc.subjectV Crateris-
dc.subjectJapal-Rangapur Observatory-
dc.titlePhotoelectric observations of V Craterisen
dc.typeArticleen
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