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Bow Shock Induced Star Formation in the LMC

Published online by Cambridge University Press:  25 May 2016

K.S. de Boer ,
J. M. Braun ,
A. Vallenari  and
U. Mebold
K.S. de Boer
Affiliation:
Sternwarte, University of Bonn, D-53121 Bonn, Germany
J. M. Braun
Affiliation:
Sternwarte, University of Bonn, D-53121 Bonn, Germany
A. Vallenari
Affiliation:
Osservatorio Astronomico, Vic. Osserv. 5, I-35122 Padova, Italy
U. Mebold
Affiliation:
Radioastronomisches Institut, Univ. Bonn, D-53121 Bonn, Germany

Extract

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The supergiant shell LMC 4 is known for its ring of HII regions and the deep minimum in HI in the interior (Rohlfs et al. 1984). LMC 4 shows X-ray emission detected by ROSAT and highly ionised gas (C IV) detected with HST (Bomans et al. 1994, 1996). The velocities of its neutral gas indicate it cannot have been formed by the collision with a high velocity cloud (Domgörgen et al. 1995).

Type
Part 6. Stellar Clusters
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 456 - 457
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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