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Detection and Photometry of Red Giants in the Magellanic Clouds

Published online by Cambridge University Press:  04 August 2017

Marc Aaronson
Marc Aaronson*
Affiliation:
Steward Observatory, University of Arizona

Abstract

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This review will focus on photometric observations of evolved stars in the Magellanic Clouds. Emphasis is placed on red and near-infrared measurements, as these allow reasonable estimates to be made of bolometric magnitude and temperature for reliable placement in the physical HR diagram. The review is divided into three parts: field stars, cluster stars, and red variables; a summary of the surveys for objects in each of these areas is also given. Particular attention is drawn to the intermediate-age stellar population, as this component appears to be the primary tracer of the star formation rate and chemical enrichment history of the Clouds.

Type
Stellar Populations
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 183 - 194
Copyright
Copyright © Reidel 1984 

References

Aaronson, M., and Mould, J.: 1982, Ap. J. Suppl., 48, 161.Google Scholar
Arp, H. C.: 1958, A. J., 63, 273.Google Scholar
Azzopardi, M., and Vineau, J.: 1975, Astr. Ap. Suppl., 22, 285.Google Scholar
Bappu, M. K. V., Parthasarathy, M., and Searia, K. K.: 1978, Kodaikanal Obs. Bull., Ser. A., 2, 184.Google Scholar
Bessell, M. S., and Wood, P. R.: 1983, M.N.R.A.S., 202, 31p.Google Scholar
Bessell, M. S., Wood, P. R., and Lloyd-Evans, T.: 1981, Proc. A.S.A., 4, 201.Google Scholar
Bessell, M. S., Wood, P. R., and Lloyd-Evans, T.: 1983, M.N.R.A.S., 202, 59.Google Scholar
Blanco, B. M., Blanco, V. M., and McCarthy, M. F.: 1978, NATURE, 271, 638.Google Scholar
Blanco, V. M., Frogel, J. A., and McCarthy, M. F.: 1981, Pub. A.S.P., 93, 532.Google Scholar
Blanco, V. M., and McCarthy, M. F.: 1983, preprint.Google Scholar
Blanco, V. M., McCarthy, M. F., and Blanco, B. M.: 1980, Ap. J., 242, 938.Google Scholar
Blanco, V. M., and Richer, H. B.: 1979, P.A.S.P., 91, 659.Google Scholar
Butcher, H.: 1977, Ap. J., 216, 372.Google Scholar
Catchpole, R. M., and Feast, M. W.: 1981, M.N.R.A.S., 197, 385.Google Scholar
Cohen, J. G., Frogel, J. A., Persson, S. E., and Elias, J. H.: 1981, Ap. J., 249, 481.Google Scholar
Crabtree, P. R., Richer, H. B., and Westerlund, B. E.: 1976, Ap. J. Letters), 203, L81.Google Scholar
Danks, A. C.: 1982, Astr. Ap., 106, 4.Google Scholar
de Boer, K. S.: 1981, in IAU Coll. No. 68, “Astrophysical Parameters for Globular Clusters”, eds. Philip, A. G. D. and Hayes, D. S. (Schenectady: L. Davis Press), p. 3.Google Scholar
de Vaucouleurs, G.: 1957, A. J., 62, 69.Google Scholar
Elias, J. H.: 1982, private communication.Google Scholar
Elias, J. H., Frogel, J. A., and Humphreys, R. M.: 1980, Ap. J. (Letters), 242, L13.Google Scholar
Feast, M. W.: 1973, in IAU Symp. No. 59, “Stellar Instability and Evolution”, eds. Ledoux, P., Noels, A., and Rodgers, A. W. (Dordrecht: Reidel), p. 93.Google Scholar
Feast, M. W.: 1981, in “The Most Massive Stars”, eds. D'odorico, S., Baade, D., and Kjar, K. (Garching: ESO), p. 217.Google Scholar
Feast, M. W., Catchpole, R. M., Carter, B. S., and Roberts, G.: 1980, M.N.R.A.S., 193, 377.Google Scholar
Feast, M. W., and Lloyd-Evans, T.: 1973, M.N.R.A.S., 164, 15p.Google Scholar
Frogel, J. A.: 1983, Ap. J., 272, 116.Google Scholar
Frogel, J. A., and Blanco, V. W.: 1983a, preprint.Google Scholar
Frogel, J. A., and Blanco, V. W.: 1983b, presented at IAU Symp. No. 105, “Observational Tests of Stellar Evolution Theory”.Google Scholar
Frogel, J. A., and Cohen, J. G.: 1982, Ap. J., 253, 580.Google Scholar
Frogel, J. A., Persson, S. E., and Cohen, J. G.: 1980, Ap. J., 239, 495.Google Scholar
Frogel, J. A., and Richer, H. B.: 1983, Ap. J., in press.Google Scholar
Glass, I. S.: 1979, M.N.R.A.S., 186, 317.Google Scholar
Glass, I. S., and Feast, M. W.: 1982, M.N.R.A.S., 199, 245.Google Scholar
Glass, I. S., and Lloyd-Evans, T.: 1981, NATURE, 291, 303.Google Scholar
Humphreys, R. M.: 1984, in IAU Symp. No. 108, “Structure and Evolution of the Magellanic Clouds”, this volume, p. 145.Google Scholar
Iben, I.: 1982, Ap. J., 260, 821.Google Scholar
Lloyd-Evans, T.: 1975, in “Variable Stars and Stellar Evolution”, eds. Sherwood, V. and Plaut, L. D. (Doredrecht: Reidel), p. 531.Google Scholar
Lloyd-Evans, T.: 1978a, M.N.R.A.S., 183, 305.Google Scholar
Lloyd-Evans, T.: 1978b, M.N.R.A.S., 183, 319.Google Scholar
Lloyd-Evans, T.: 1980, M.N.R.A.S., 193, 87.Google Scholar
Lloyd-Evans, T.: 1983a, M.N.R.A.S., in press.Google Scholar
Lloyd-Evans, T.: 1983b, M.N.R.A.S., submitted.Google Scholar
Lloyd-Evans, T.: 1984, presented at IAU Symp. No. 108, “Structure and Evolution of the Magellanic Clouds”, this volume, p. 217.Google Scholar
Mendoza, E. E., and Gomez, T.: 1973, Pub. A.S.P., 85, 439.Google Scholar
Mould, J. R.: 1984 in IAU Symp. No. 108, “Structure and Evolution of the Magellanic Clouds”, this volume, p. 195.Google Scholar
Mould, J., and Aaronson, M.: 1979, Ap. J., 232, 421.Google Scholar
Mould, J., and Aaronson, M.: 1980, Ap. J., 240, 464.Google Scholar
Mould, J., and Aaronson, M.: 1982, Ap. J., 263, 629.Google Scholar
Paltoglou, G., Wood, P. R., and Bessell, M. S.: 1984, presented at IAU Symp. No. 108, “Structure and Evolution of the Magellanic Clouds”, this volume, p. 219.Google Scholar
Payne-Gaposchkin, C. H.: 1971, Smith Contr. Ap., No. 13.Google Scholar
Payne-Gaposchkin, C.H., and Gaposchkin, S.: 1966, Smith. Contr. Ap., No. 9.Google Scholar
Persson, S. E., Aaronson, M., Cohen, J. G., Frogel, J. A., and Matthews, K.: 1983, Ap. J., 266, 105.Google Scholar
Prévot, L., Martin, N., Maurice, E., Rebeirot, E., and Rousseau, J.: 1983, Astr. Ap. Suppl., 53, 255.Google Scholar
Rabin, D.: 1982, Ap. J., 261, 85.Google Scholar
Rebeirot, E., Martin, N., Miares, P., Prévot, L., Robin, A., Rousseau, J., and Peyrin, Y.: 1983, Astr. Ap, Suppl., 51, 277.Google Scholar
Reid, N.: 1983, privately communicated by Glass, I. S. Google Scholar
Reid, N., and Mould, J. R.: 1983, in preparation.Google Scholar
Richer, H. B.: 1981, Ap. J., 243, 744.Google Scholar
Richer, H. B., and Frogel, J. A.: 1980, Ap. J. (Letters), 242, L9.Google Scholar
Richer, H. B., Olander, N., and Westerlund, B. E.: 1979, Ap. J., 230, 724.Google Scholar
Richer, H. B., and Westerlund, B. E.: 1983, Ap. J., 264, 114.Google Scholar
Ridgway, S. T., Jacoby, G. H., Joyce, R. R., and Wells, D. C.: 1980, in IAU Coll. No. 59, “Physical Processes in Red Giants”, eds. Iben, I. and Renzini, A. (Dordrecht: Reidel), p. 47.Google Scholar
Sanduleak, N.: 1975, Astr. Ap., 39, 461.Google Scholar
Sanduleak, N., and Philip, A. G. D.: 1977, Pub. Warner Swasey Obs., 2, No. 5.Google Scholar
Searle, L., Wilkinson, A., and Bagnuolo, N.: 1980, Ap. J., 239, 803.Google Scholar
Stryker, L., and Butcher, H.: 1981, in IAU Coll. No. 68, “Astrophysical Parameters for Globular Clusters”, eds. Philip, A. G. D. and Hayes, D. S. (Schnectady: L. Davis Press), p. 255.Google Scholar
Tifft, W. G., and Snell, C. M.: 1971, M.N.R.A.S., 151, 365.Google Scholar
van den Bergh, S.: 1981, Astr. Ap. Suppl., 46, 79.Google Scholar
Walker, M. F., Blanco, V. M., and Kunkel, W. E.: 1969, A. J., 74, 44.Google Scholar
Westerlund, B. E.: 1983, private communication.Google Scholar
Westerlund, B. E., Olander, N., and Hedin, B.: 1981, Astr. Ap. Suppl., 43, 267.Google Scholar
Westerlund, B. E., Olander, N., Richer, H. B., and Crabtree, D. R.: 1978, Astr. Ap. Suppl., 31, 61.Google Scholar
Wood, P. R.: 1981, in IAU Coll. No. 59, “Physical Processes in Red Giants”, eds. Iben, I. and Renzini, A. (Dordrecht: Reidel), p. 135.Google Scholar
Wood, P. R., Bessell, M. S., and Fox, M. W.: 1981, Proc. A.S.A., 4, 203.Google Scholar
Wood, P. R., Bessell, M. S., and Fox, M. W.: 1983, Ap. J., 272, 99.Google Scholar