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CCD and Schmidt-Plate Photometry and Astrometry in Region E of the LMC

Published online by Cambridge University Press:  26 July 2016

D.J. Bomans ,
H.-J. Tucholke ,
J.-M. Will  and
K.S. de Boer
D.J. Bomans
Affiliation:
Sternwarte der Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
H.-J. Tucholke
Affiliation:
Sternwarte der Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany Astronomisches Institut, Universität Münster
J.-M. Will
Affiliation:
Sternwarte der Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
K.S. de Boer
Affiliation:
Sternwarte der Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany

Extract

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Shapley Constellation III in the north of the LMC is one of the largest associations in the LMC. It is surrounded by a ring of H II regions and diffuse H II filaments called Supergiant Shell LMC 4 (Goudis & Meaburn 1978). LMC 4 is suspected to be a site of large scale propagation of star formation (Dopita et al. 1985), but recent studies (Reid et al. 1987; Vallenari et al. 1993) show that the situation is far from simple.

Type
Part Ten: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 520 - 522
Copyright
Copyright © Kluwer 1994 

References

Bastian, U., Röser, S., et al., 1991. Astron. Astrophys. Suppl., 87, 159.Google Scholar
Bomans, DJ., Tucholke, H.-J., Vallenari, A., de Boer, K.S., Grebel, E.K., Richtler, T. and Seggewiss, W., 1993. In preparation.Google Scholar
de Boer, K.S., et al., 1991. ESO Messenger, 66, 14.Google Scholar
de Boer, K.S., 1992. In ‘New Aspects of Magellanic Cloud Research’, eds. Baschek, B., Klare, G., Lequeux, J., Springer, p. 389.Google Scholar
Dopita, M.A., Mathewson, D.S. and Ford, V.L., 1985. Astrophys. J., 297, 599.Google Scholar
Goudis, C. and Meaburn, J., 1978. Astron. Astrophys., 68, 169.Google Scholar
Hatzidimitriou, D., Hawkins, M.R.S. and Gyldenkerne, K., 1989. Mon. Not. R. astron. Soc., 241, 645.Google Scholar
Reid, I.N., Mould, J. and Thompson, I., 1987. Astrophys. J., 323, 433.Google Scholar
Taff, L.G., Lattanzi, M.G. and Bucciarelli, B., 1990. Astrophys. J., 358, 359.Google Scholar
Tucholke, H.-J. and Hiesgen, M. 1991. In: IAU Symp. 148, ‘The Magellanic Clouds’, eds. Haynes, R., Milne, D., Kluwer, p. 491.Google Scholar
Vallenari, A., Bomans, DJ. and de Boer, K.S., 1993. Astron. Astrophys., 268, 137.Google Scholar