Proceedings of the Workshop
"The Magellanic Clouds and Other Dwarf Galaxies"
of the Bonn/Bochum-Graduiertenkolleg

ROSAT observations of the giant

H II complex N 11 in the LMC

Mordecai-Mark Mac Low, Thomas H. Chang, You-Hua Chu,

Sean D. Points, R. Chris Smith, and Bart P. Wakker

 [Fig. 1]
Fig. 1. Contours of X-ray emission superimposed on our Curtis Schmidt Halpha image. This X-ray image was derived by binning the PSPC image by a factor of 8 and smoothed by a gaussian of σ=8". The contours are 10%, 13%, 16%, and 20% of the peak brightness of the supernova remnant N 11 L at 04h 54m 48.5s, -66° 25' 45". The RA and DEC are in J2000. The source and background regions are marked
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First version: 09thAugust,1998
Last update: 30thSeptember,1998
Jochen M. Braun   &   Tom Richtler
 (E-Mail: jbraun|richtler@astro.uni-bonn.de)