No CrossRef data available.
Article contents
Two-Dimensional Spectral Classification of M Stars by Narrow-Band Photometry
Published online by Cambridge University Press: 14 August 2015
Extract
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.
To place a star on the HR diagram by means of spectroscopic data alone-i.e., without knowledge of the parallax-one must separate the spectroscopic effects of temperature and luminosity as cleanly as possible. Here we discuss the use of the red and near-infrared bands of TiO, VO, CN, and CaH as classification criteria for M stars. Our eight-color system of filter photometry (Wing 1971; White 1971a) has provided data on the first three molecules.
- Type
- Poster Session
- Information
- Copyright
- Copyright © Reidel 1978
References
Keenan, P.C. (1963). In Basic Astronomical Data, Strand, K. Aa., ed., Univ. of Chicago Press, Chicago, p. 78.Google Scholar
White, N.M. (1971a). In Proceedings of the Conference on Late-Type Stars, Lockwood, G.W. and Dyck, H.M., eds. (KPNO Contr. No. 554), p. 163.Google Scholar
Wing, R.F. (1971). In Proceedings of the Conference on Late-Type Stars, Lockwood, G.W. and Dyck, H.M., eds. (KPNO Contr. No. 554), p. 145.Google Scholar
Wing, R.F. (1973a). In Spectral Classification and Multicolor Photometry, Fehrenbach, Ch. and Westerlund, B.E., eds., D. Reidel, Dordrecht, p. 209.Google Scholar
You have
Access