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A Deep Survey of Infrared Sources in the Field of the Small Magellanic Cloud

Published online by Cambridge University Press:  25 April 2016

S. C. Russell  and
A. R. Hyland
S. C. Russell
Affiliation:
Mount Stromlo and Siding Spring Observatories, Australian National University
A. R. Hyland
Affiliation:
Mount Stromlo and Siding Spring Observatories, Australian National University
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Abstract

We present a survey at J (1.25μm) and K (2.2μm) of 36 arcmin2 in the Bar and Inner Wing of the Small Magellanic Cloud. The (J-K) colour – bolometric magnitude diagram is constructed and compared with theory. For the first time a sparsely populated region of the diagram separating proposed carbon stars from oxygen rich stars has been identified. In addition large numbers of red sources have been found apparently fainter than the accepted limit for carbon star formation. These include extremely red sources which are good candidates for OH/IR sources and extreme carbon stars.

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Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 1 , 1985 , pp. 52 - 54
Copyright
Copyright © Astronomical Society of Australia 1985

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References

Allen, D. A., Hyland, A. R., Longmore, A. J., Caswell, J. L., Goss, W. M. and Haynes, R. F., 1977, Astrophys, J., 217, 108.Google Scholar
Basinski, J. M., Bok, B. J., and Bok, P. F., 1967, Mon. Not. R. Astron. Soc., 137, 55.Google Scholar
Becker, S. A., and Iben, I. Jr., 1979, Astrophys. J., 232, 831.Google Scholar
Becklin, E. E., Frogel, J. A., Hyland, A. R., Kristian, J., Neugebauer, G., 1969, Astrophys. J. Lett., 158, L133.Google Scholar
Bessell, M. S., Wood, P. R., and Evans, L. T., 1983, Mon. Not. R. Astron. Soc., 202, 59.Google Scholar
Blanco, V. M., and McCarthy, M. F., 1983, Astron. J., 88, 1442 Google Scholar
Blanco, V. M., and McCarthy, M. F., 1981, ‘Physical Processes in Red Giants’, ed. Iben, I. Jr. and Renzini, A. (Dordrect: Reidel) p. 147.Google Scholar
Blanco, V. M., McCarthy, M. F., and Blanco, B. M., 1980, Astrophys. J., 242, 938.Google Scholar
Casswell, J. L., and Haynes, R. F., 1975, Mon. Not. R. Astron. Soc., 173, 649.Google Scholar
Cohen, J. G., Frogel, J. A., Persson, S. E., and Elias, J. H., 1981, Astrophys. J., 249, 481.Google Scholar
Frogel, J. A., and Richer, H. B., 1983, Astrophys. J., 275, 84.Google Scholar
Hardy, E., and Durand, D., 1984, Astrophys. J., 279, 567.Google Scholar
Hyland, A. R., Becklin, E. E., Frogel, J. A., and Neugebauer, G., 1972, Astron. Astrophys., 16, 204.Google Scholar
Iben, I. Jr., 1975, Astrophys. J., 196, 525.Google Scholar
Iben, I. Jr., and Renzini, A., 1982, Astrophys. J. Lett., 259, L79.Google Scholar
Iben, I. Jr., and Renzini, A., 1983, Annu. Rev. Astron. Astrophys., 21, 271.Google Scholar
Jones, T. J., Hyland, A. R., Caswell, J. L., and Gatley, I., 1982, Astrophys. J., , 253, 208.Google Scholar
Jones, T. J., Hyland, A. R., Wood, P. R., and Gatley, I., 1983, Astrophys. J., 273, 669.Google Scholar
Lance, K., and Hyland, A. R., 1983, private communication.Google Scholar
Mathewson, D. S., 1985, Proc. Astron. Soc., 6, 104.Google Scholar
Ruelas-Mayorga, A., 1982, Thesis.Google Scholar
Schwarzschild, M., and Harm, R., 1965, Astrophys. J., 142, 855 Google Scholar
Wood, P. R., Bessell, M. S., and Fox, M. W., 1983, Astrophys. J., 272, 99 Google Scholar