Ultraluminous IRAS Galaxies as seen with ISO

Rigopoulou, D; Genzel, R; Lutz, D; Kunze, D; Moorwood, AFM; Spoon, HWW; Sturm, E; Thornley, M; Tran, D

Abstract:

We review the results of a major spectroscopic survey of nearby Starbursts and moderate redshift Ultraluminous IRAS Galaxies (ULIRGs) using ISO-SWS, ISOPHOT-S and ISOCAM (CVF) on board ISO. Detailed modeling reveals that massive stars, M-upper greater than or equal to 100 M-. are formed in most Starbursts in relatively short bursts (one or a few O star lifetimes). In the area of ULIRGs we address the main question of the dominant energy source as well as their evolution. We have found that th...

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APA Style

Rigopoulou, D., Genzel, R., Lutz, D., Kunze, D., Moorwood, A. F. M., Spoon, H. W. W., Sturm, E., Thornley, M., & Tran, D. (1999). Ultraluminous IRAS Galaxies as seen with ISO. 427, 833–838.

MLA Style

Rigopoulou, D., et al. Ultraluminous IRAS Galaxies as Seen with ISO. 1999, pp. 833–38.

Chicago Style

Rigopoulou, D, R Genzel, D Lutz, D Kunze, AFM Moorwood, HWW Spoon, E Sturm, M Thornley, and D Tran. 1999. “Ultraluminous IRAS Galaxies as Seen with ISO.” In , 427:833–38.
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