The Magellanic Cloud
Emission Line Survey:
Image Gallery

Here you can see a selection of the beautiful emission-line images of various nebulae in the Magallanic Clouds which we are obtaining in the Magellanic Cloud Emission Line Survey. (NOTE: images are not presented in the same spatial scale)


N9 and N4 Three nebular complexes in the Large Magellanic Cloud. To the left is N9 (the large loop), in the lower right is N5, and in the upper right is N4 complex. The image is combination of images made in three filters: Halpha emission, green is [SII], and blue is [OIII]. The greenish areas, such as the little hook just in the right edge of N9 and the large half bubble in N4, are newly identified supernova remnants.
(Smith et al., 1994, AJ, 108, 1266)

N44 This is the region N44. Here, red is Halpha emission, green is [SII], and blue is [OIII]. Notice the green area to the upper-left in the image. This is a previously undetected (at least optically) supernova remnant!
( Kim et al., 1998, ApJ, 503, 729)

Image selected as the Astronomy Picture of the Day, 1996 July 3.


dem192 DEM 192. In this image, red is Halpha emission, green is [SII], and blue is [OIII]
(Oey & Smedley, 1998, AJ, 116, 1263)

Image selected as the Astronomy Picture of the Day, 1996 June 25 and 1997 August 23.


The superbubble LMC 2 in the combined light of hydrogen, sulfur and oxigen.
(Points, S. D. et al., 1999, ApJ, 518, 298. )

Image selected as the Astronomy Picture of the Day, 1997 July 25 .


Colliding Remnants DEM L316.
(Williams et al., 1997, ApJ, 480, 618)

Image selected as the Astronomy Picture of the Day, 1997 October 2.


The giant HII complex 30 Doradus in the combined light of hydrogen, sulfur and oxigen.

Image selected as the Astronomy Picture of the Day, 2005 December 12


Superbubble N11.
(MacLow, M. et al., 1998, ApJ, 493, 260)

Image selected as the Astronomy Picture of the Day, 2004 October 6



The MCELS project has been supported in part by NSF grants AST-9540747 and AST-0307613, and through the generous support of the Dean B. McLaughlin Fund at the University of Michigan, a bequest from the family of Dr. Dean B. McLaughlin in memory of his lasting impact on Astronomy. The National Optical Astronomy Observatory is operated by the Association of Universities for Research in Astronomy Inc. (AURA), under a cooperative agreement with the National Science Foundation.

This Web page is maintained by Chris Smith and Roger Leiton at Cerro Tololo Inter-American Observatory. Please send comments, suggestions, or reports of any problems to csmith@ctio.noao.edu.

Last update: January 9, 2006 by RCS