No CrossRef data available.
Article contents
Secondary Spectrophotometric Standards: Results and Future Observational Programme
Published online by Cambridge University Press: 12 April 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Three sets of spectrophotometric standards are presented: eight bright B and A stars of 00 - 265, fourteen B - A stars of 3m-4m from the catalogue of 238 secondary spectrophotometric standards and 24 A0-G0 stars of 7m-8m. For all of these stars UBV photometry was produced and brightness variations exceeding O01 were not found.
- Type
- Session 2 High Precision Photometry
- Information
- Copyright
- Copyright © C.J. Butler and I. Elliottt 1993
References
Glushneva, I.N.
1992 in: Proceedings of a Joint Meeting of Comm. 9 and 25, 21st General Assembly PASP Conference Ser., Ed. Adelman, S.J. and Dukes, J. Jr., in press.Google Scholar
Hayes, D.S.
1985, Calibration of Fundamental Stellar Quantities, in IAU Symposium 111, Eds. Hayes, D.S., Passinetti, L.E. and Philip, A.G.Davis, p.247.Google Scholar
Kharitonov, A.V.
et al.
1988, Spectrophotometricheskij Katalog Zvezd, Alma-Ata, Nauka.Google Scholar
Nesterov, V.V.
et al.
1990, Inertial Coordinate System on the Sky in: IAU Symp. 141, Eds. Lieske, J.H. and Abalakin, V.K., p.355.CrossRefGoogle Scholar
Voloshina, I.B.
et al.
1982, Spectrophotometry of Bright Stars, Ed. Glushneva, I.N. (Nauka Publ., Moscow), 255 pp.Google Scholar
You have
Access