Results 141 to 150 of about 629 (178)
Fe K emission in the ultraluminous infrared galaxy Arp 220 [PDF]
K. Iwasawa +5 more
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Molecular gas inflows and outflows in ultraluminous infrared galaxies at z ∼ 0.2 and one QSO at z = 6.1 [PDF]
R. Herrera-Camus +14 more
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COMPLEX RADIO SPECTRAL ENERGY DISTRIBUTIONS IN LUMINOUS AND ULTRALUMINOUS INFRARED GALAXIES [PDF]
Adam K. Leroy +13 more
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Extinction law in ultraluminous infrared galaxies at z∼ 1 [PDF]
Thomas Shimizu +5 more
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Is HCN a True Tracer of Dense Molecular Gas in Luminous and Ultraluminous Infrared Galaxies? [PDF]
J. Graciá-Carpio +3 more
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Far-Infrared Line Deficits in Ultraluminous Infrared Galaxies
SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan We study the origin of the [O I] 63, [N II] 122, [O I] 145, and [C II] 158 line deficits in z less than 0.3 Ultraluminous Infrared Galaxies, using data from Herschel.
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SUZAKU OBSERVATIONS OF LOCAL ULTRALUMINOUS INFRARED GALAXIES
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Star formation in the local environments of high-redshift ultraluminous infrared galaxies [PDF]
E. N. Dubois
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Ultraluminous Infrared Galaxies at 1.5
2007We present measurements of the spatial clustering of ultraluminous infrared galaxies in two redshift intervals, 1.51.
Farrah, D. +11 more
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