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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

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