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Peculiar Red Giants in External Galaxies

Published online by Cambridge University Press:  12 April 2016

Harvey B. Richer*
Affiliation:
University of British Columbia, Vancouver, B.C. V6T 1W5, Canada

Abstract

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Study of the late-type stellar content in external galaxies provides numerous clues for the theory of stellar evolution, for star-formation scenarios in galaxies, and for proper models of the luminosity evolution of galaxies which are then used in cosmological studies. In addition, these late-type stars can be used as distance indicators themselves and yield a local value of the Hubble constant consistent with recent Cepheid determinations.

Type
1. Properties and Kinematics of the Peculiar Red Giant Stars
Copyright
Copyright © Cambridge University Press 1989

References

Aaronson, M., and Mould, J.R. 1985, Ap.J., 290, 191.Google Scholar
Aaronson, M. , Mould, J.R., and Huchra, J. 1980, Ap.J., 237, 655.Google Scholar
Azzopardi, M., Lequeux, J., and Westerlund, B.E. 1985, Astr. Ap., 144. 388.Google Scholar
Blanco, V.M., Blanco, B.M., and McCarthy, M.F. 1978, Nature, 271, 638.Google Scholar
Blanco, V.M., McCarthy, M.F., and Blanco, B.M. 1980, Ap.J., 242, 938.Google Scholar
Blanco, V.M., and McCarthy, M.F. 1983, A.J., 88, 1442.Google Scholar
Chokshi, A., and Wright, E.L. 1987, Ap.J., 319, 44.Google Scholar
Cook, K.H., Aaronson, M. , and Norris, J. 1986, Ap.J., 305., 634.Google Scholar
Djorgovski, S., Splnrad, H., and Marr, J. 1985, in New Aspects of Galaxy Photometry, ed. J.L. Nieto (Lecture Notes in Physics, 232). p. 193.Google Scholar
Frogel, J.A., Cohen, J.G., Persson, S.E., and Elias, J.H. 1981, in Physical Processes in Red Giants, eds Iben, I. Jr., and Renzini, A. (Dordrecht: Reidel), p. 159.Google Scholar
Frogel, J.A., and Richer, H.B. 1983, Ap.J., 275, 84.Google Scholar
Hudon, D., and Richer, H.B. 1989, in preparation.Google Scholar
Iben, I. Jr. and Renzini, A. 1983, Ann. Rev. Astr. Ap. 21, 271.Google Scholar
Lattanzio, J.C. 1986a, Ap.J., 311, 708.Google Scholar
Lattanzio, J.C. 1986b, in Calgary Workshop on Late Stages of Stellar Evolution, ed. Kwok, S. and Pottasch, S.R., (Dordrecht: Reidel), p. 235.Google Scholar
Lattanzio, J.C. 1987, Ap.J. (Letters), 313, 15.Google Scholar
Lilly, S.J. 1987, M.N.R.A.S., 222, 573.Google Scholar
Pritchet, C.J., Richer, H.B., Schade, D., Crabtree, D., andYee, H.K.C. 1987, Ap.J., 123, 79.Google Scholar
Reid, N., and Mould, J.R. 1984, Ap.J., 284. 98.Google Scholar
Renzini, A., and Voli, M. 1981, Astr. Ap., 94, 175.Google Scholar
Richer, H.B. 1981a, Ap.J., 243, 744.Google Scholar
Richer, H.B. 1981b, in Physical Processes in Red Giants, ed. I. Iben Jr. , and Renzini, A. (Dordrecht: Reidel) , p. 153.Google Scholar
Richer, H.B., and Crabtree, D.R. 1985, Ap.J. (Letters), 198, L13.Google Scholar
Richer, H.B., Crabtree, D.R., and Pritchet, C.J. 1984, Ap.J., 287. 138.Google Scholar
Richer, H.B., Pritchet, C.J., and Crabtree, D.R. 1985, Ap.J., 298. 240.Google Scholar
Sanduleak, N., and Phillip, A.G.D. 1977, Pub. Warner and Swasey Observatory, Vol. 2, No. 5, p. 105.Google Scholar
Tulley, R.B., and Fisher, J.R. 1977, Astr. Ap., 54, 661.Google Scholar
Van den Bergh, S. 1984, Q. Jour. R. Ast. Soc, 25, 137.Google Scholar
Welch, D.L., McAlary, C.W., McLaren, R.A., and Madore, B.F. 1984, in IAU Colloquium 82, Cepeids: Observations and Theory, ed. Madore, B.F. (New York: Cambridge University Press), p. 219.Google Scholar
Westerlund, B.E. 1960, Uppsala Astron. Obs. Ann., 4, No. 7.Google Scholar
Westerlund, B.E. 1964, M.N.R.A.S., 127, 429.Google Scholar
Westerlund, B.E. 1965, M.N.R.A.S., 130, 45.Google Scholar
Westerlund, B.E., Olander, N. , Richer, H.B., andCrabtree, D.R. 1978, Astr. Ap. (Suppl.), 11, 61.Google Scholar
Wing, R.F. 1971, in Proceedings of the Conference on Late-Type Stars, eds. G.W. Lockwood and H.M. Dyck (KPNO Contr. No. 554), p.145.Google Scholar