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The Absolute Calibration of the HR Diagram: Fundamental Effective Temperatures and Bolometric Corrections

Published online by Cambridge University Press:  14 August 2015

D. S. Hayes*
Affiliation:
Arizona State University

Extract

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Scales of fundamental bolometric connections (B.C.) and effective temperatures (Teff) as a function of spectral type or color are necessary for the comparison of observations and theory in the HR diagram.

Type
Part I: Fundamentals of the HR Diagram
Copyright
Copyright © Reidel 1978 

References

Barnes, T. G. and Evans, D. S. (1976). Mon. Not. R. Astron. Soc. 174, 489.Google Scholar
Blazit, A., Bonneau, D., Josse, M., Koechlin, L. and Labeyrie, A. (1977). Astrophys. J. Lett., 214, L79.Google Scholar
Code, A.D., Davis, J., Bless, R.C. and Hanbury Brown, R. (1976). Astrophys. J., 203, 417.Google Scholar
Conti, P. S. (1973). Astrophys. J., 179, 181.Google Scholar
Currie, D. G., Knapp, S. L. and Liewer, K. M. (1974). Astrophys. J., 187, 131.Google Scholar
Forgan, B. W. (1977). Appl. Optics, 16, 1628.Google Scholar
Frogel, J. A., Kleinman, D. E., Kunkel, W., Ney, E. P. and Strecker, D. W. (1972), Publ. Astron. Soc. Pacific, 84, 581.Google Scholar
Gallouët, L. (1964). Ann. d'Astrophys., 27, 423.Google Scholar
Gezari, D. Y., Labeyrie, A. and Stachnik, R. V. (1972). Astrophys. J. Lett., 173, L1.Google Scholar
Greenstein, J. L., Neugebauer, G., and Becklin, E. E. (1970). Astrophys. J., 161, 519.Google Scholar
Hanbury Brown, R. (1968). In Ann. Rev. Astron. Astrophys., Vol. 6, Annual Reviews, Palo Alto, p. 13.Google Scholar
Harris, D. L. III (1963). In Stars and Stellar Systems, Vol. III, Basic Astronomical Data, Strand, K. Aa., ed., University of Chicago Press, Chicago, p. 263.Google Scholar
Hayes, D. S. (1970). In IAU Symposium No. 36, Ultraviolet Stellar Spectra and Related Ground-Based Observations, Houziaux, L. and Butler, H. E., eds., D. Reidel, Dordrecht, p. 83.Google Scholar
Hayes, D. S. and Latham, D. W. (1975). Astrophys. J., 197, 593.Google Scholar
Johnson, H. L. (1965). Comm. Lunar Planet. Lab., No. 53, 73.Google Scholar
Johnson, H. L. (1966). In Ann. Rev. Astron. Astrophys., Vol. 4, Annual Reviews, Palo Alto, p. 193.Google Scholar
Kuiper, G. P. (1938). Astrophys. J., 88, 429.Google Scholar
Mould, J. R. and Hyland, A. R. (1976). Astrophys. J., 208, 399.Google Scholar
Oke, J. B. and Schild, R. E. (1970). Astrophys. J., 161, 1015.Google Scholar
Panagia, N. (1973). Astron. J., 78, 929.CrossRefGoogle Scholar
Popper, D. M. (1959). Astrophys. J., 129, 647.Google Scholar
Ridgway, S. T., Wells, D. C. and Joyce, R. R. (1977). Astron. J., 82, 414.Google Scholar
Stebbins, J. and Kron, G. (1957). Astrophys. J., 126, 266.Google Scholar
Tug, H., White, N. M. and Lockwood, G. W. (1977). Astron. Astrophys. in press.Google Scholar
Veeder, G. J. (1974). Astron. J., 79, 1056.Google Scholar
Vilas, F. and Lasker, B. M. (1977). Publ. Astron. Soc. Pacific, 89, 95.Google Scholar
Walker, R. G. (1969). Phil. Trans. Roy. Soc. London, A, 264, 209.Google Scholar
Worden, S. P. (1976). Publ. Astron. Soc. Pacific, 88, 69.Google Scholar