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Criteria and Applications of the MK Classification System

Published online by Cambridge University Press:  12 April 2016

R. F. Garrison*
Affiliation:
David Dunlap Observatory, University of Toronto

Abstract

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A review is given of the present state of MK classification, with a view to future developments in techniques and instrumentation. The principle of the complementarity of quantitative and visual inspection techniques is stressed.

Included in the discussion are examples of problems which are currently outstanding. Among these are variable stars, marginal peculiarities, fundamental standards (with specific reference to the Sun), and representation of the third and higher dimensions.

Type
II Criteria and Applications of MK Classification
Copyright
Copyright © Vatican Observatory 1979

References

Barry, D.C., Cromwell, R.H. and Schoolman, S.A. (1978). Astrophys. J. 222, 1032.CrossRefGoogle Scholar
Code, A.D. (1947). Astrophys. J. 106, 309.CrossRefGoogle Scholar
Croft, S.K., McNamara, D.H. and Feltz, K.A. (1972). Publ. Astron. Soc. Pacific 84, 515.CrossRefGoogle Scholar
Fernie, J.D., Hagen, J.P., Hagen, G.L. and McClure, L. (1971). Publ. Astron. Soc. Pacific 83., 79.CrossRefGoogle Scholar
Hardorp, J. (1978). Astron. and Astrophys. 63, 383.Google Scholar
Keenan, P.C., Garrison, R.F. and Deutsch, A.J. (1974). Astrophys. J. Supp. 28, 271.CrossRefGoogle Scholar
Reitsema, H.J. (1977). Bull. Astron. and Astrophys. Soc. 9, 635.Google Scholar
Stehbins, J. and Kron, G.E. (1957). Astrophys. J. 126. 266.CrossRefGoogle Scholar