Bournaud, F., Daddi, E., Elmegreen, B. G., Elmegreen, D. M., Nesvadba, N., Vanzella, E., ...
We investigate the properties of a clump-cluster galaxy at redshift 1.57. The morphology of this galaxy is dominated by eight star-forming clumps in optical observations, and has photometric...
Hunter, D. A., Elmegreen, B. G., Dupuy, T. J., Mortonson, M.
The properties of 939 star clusters in the Large and Small Magellanic Clouds were determined from ground-based CCD images in UBVR passbands. The areal coverage was extensive, corresponding to 11.0...
6-m Telescope Spectroscopic Observations of the Bubble Complex in NGC 6946 (2002)
Efremov, Yu. N., Pustilnik, S. A., Kniazev, A. Y., Elmegreen, B. G., Larsen, S. S., Alfaro, E. J., ...
Efremov, Y. N., Elmegreen, B. G.
The average age difference between pairs of star clusters in the Large Magellanic Clouds increases with their separation as the ~0.35 power. This suggests that star formation is hierarchical in space...
The Interaction between Spiral Galaxies IC 2163 and NGC 2207. I. Observations. (1995)
Elmegreen, D.M., Kaufman, M., Brinks, E., Elmegreen, B.G., Sundin, M.
Original article can be found at: http://adsabs.harvard.edu/abs/ Copyright American Astronomical Society. DOI: 10.1086/176374 [Full text of this article is not available in the UHRA]
The Interaction between Spiral Galaxies IC 2163 and NGC 2207. II. Models. (1995)
Elmegreen, B.G., Sundin, M., Kaufman, M., Brinks, E., Elmegreen, D.M.
Original article can be found at: http://adsabs.harvard.edu/abs/ Copyright American Astronomical Society. DOI: 10.1086/176375 [Full text of this article is not available in the UHRA]