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Distribution of young stars and gas in the Small Magellanic Cloud

Published online by Cambridge University Press:  19 July 2016

J. Lequeux
J. Lequeux*
Affiliation:
Observatoire de Meudon, 92195 Meudon CEDEX, France, and Ecole Normale Supérieure

Abstract

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The relations between the distributions of interstellar gas and young stars in the central parts of the SMC are discussed, based on their distributions over the sky, radial velocities and distances. There are large differences between stars and gas. The existence of two main complexes is confirmed. There is no strong evidence for a distance in depth between these complexes larger than about 10 kpc, although Cepheid observations suggest a large total depth in some regions. Further, more accurate observations of Cepheids, especially of their mean radial velocities, are required for a better understanding of the structure of the SMC.

Type
Large-Scale Structure and Kinematics
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 25 - 29
Copyright
Copyright © Kluwer 1991 

References

Caldwell, J.A.R., Coulson, I.M. (1986), Mon. Not. R. Astron. Soc. 218, 223.Google Scholar
Feast, M. (1990), these proceedings.Google Scholar
Fitzpatrick, E.L. (1985), Astrophys. J. Suppl. Ser. 59, 77.Google Scholar
Laney, C.D., Stobie, R.S. (1986), Mon. Not. R. Astron. Soc. 222, 449.Google Scholar
Martin, N., Prévot, L., Rebeirot, E., Rousseau, J. (1976), Astron. Astrophys. 51, 31.Google Scholar
Martin, N., Maurice, E., Lequeux, J. (1989), Astron. Astrophys. 215, 219. (MML).Google Scholar
Mathewson, D.S., Ford, V.L. (1984), IAU Symp. 108 Structure and Evolution of the Magellanic Clouds , van den Bergh, S. and de Boer, K.S. (eds.) (Reidel: Dordrecht) p. 125. (MF).Google Scholar
Mathewson, D.S., Ford, V.L., Visvanathan, N. (1986), Astrophys. J. 301, 664. (MFV).CrossRefGoogle Scholar
Mathewson, D.S., Ford, V.L., Visvanathan, N. (1988), Astrophys. J. 333, 617. (MFV).Google Scholar
Maurice, E., et al. (1987), Astron. Astrophys. Suppl. Ser. 67, 423.Google Scholar
Maurice, E., Bouchet, P., Martin, N. (1989), Astron. Astrophys. Suppl. Ser. 78, 445.Google Scholar
McGee, R. X., Newton, L.M. (1981), Proc. Astron. Soc. Aust. 4, 189.Google Scholar
Prévot, L., Rousseau, J., Martin, N. (1989), Astron. Astrophys. 225, 303.Google Scholar
Rubio, M., Garay, G., Montani, J., Thaddeus, P. (1990), Astrophys. J. in preparation.Google Scholar
Tully, R.B., Wolff, S.C. (1984), Astrophys. J. 281, 67.Google Scholar
Welch, D.L., McLaren, R.A., Madore, B.F., McAlary, C.W. (1987), Astrophys. J. 321, 162. (WMMM).Google Scholar
Westerlund, B.E. (1990), Astron. Astrophys. Rev. 2, 29.Google Scholar