Results 201 to 210 of about 30,280 (240)

HSTNICMOS Imaging ofz∼ 2, 24 μm–selected Ultraluminous Infrared Galaxies [PDF]

, 2008
K. M. Dasyra, Lin Yan, G. Hélou, J. Surace, Anna Sajina, James Colbert   +5 more
openalex   +1 more source

Revealing an Energetic Galaxy-Wide Outflow in a z~2 Ultraluminous Infrared Galaxy [PDF]

, 2009
D. M. Alexander, A. M. Swinbank, Ian Smail, Richard M. McDermid, N. P. H. Nesvadba   +4 more
openalex   +1 more source

Is HCN a True Tracer of Dense Molecular Gas in Luminous and Ultraluminous Infrared Galaxies? [PDF]

, 2006
J. Graciá-Carpio, S. Garcia-Burillo, P. Planesas, L. Colina, J. Graciá-Carpio, S. Garcia-Burillo, P. Planesas, L. Colina   +7 more
openalex   +1 more source

VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies: III. the atlas of the stellar and ionized gas distribution

, 2012
J. Rodriguez-Zaurín, Santiago Arribas, A. Monreal‐Ibero, L. Colina, A. Alonso‐Herrero, J. Alfonso-Garzón   +5 more
openalex   +2 more sources

Far-Infrared Line Deficits in Ultraluminous Infrared Galaxies

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.
openaire  

Observational data analysis of Spitzer Infrared Spectrograph low-resolution spectra of ultraluminous infrared galaxies with Seyfert spectral types from the 1-Jy sample

, 2014
P. S. Chen, H. Shan
semanticscholar   +1 more source

EVOLUTIONARY PATHS ALONG THE BPT DIAGRAM FOR LUMINOUS AND ULTRALUMINOUS INFRARED GALAXIES

, 2014
S. Fiorenza, T. Takeuchi, K. Małek, Charles T. Liu   +3 more
semanticscholar   +1 more source

Star formation in the local environments of high-redshift ultraluminous infrared galaxies [PDF]

, 2015
E. N. Dubois
openalex  

From merging galaxies to quasars: The evolution of nuclear activity in luminous and ultraluminous infrared galaxies

, 2010
Stacy H. Teng
openalex   +1 more source

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Hot Dust in Ultraluminous Infrared Galaxies

Astrophysics, 2017
Ultraluminous infrared galaxies with total luminosities an order of magnitude greater than that of our galaxy over wavelengths of λλ = 10-800 μm are characterized by a high mass concentration of dust. Because of this, the optical thickness of the interstellar gas is extremely high, especially in the central regions of the galaxies, ranging from 1 at ...
Yu. A. Shchekinov, E. O. Vasiliev
openaire   +2 more sources