Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-25T04:59:16.004Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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