Results 141 to 150 of about 5,389 (174)

Interstellar H(3)(+). [PDF]

Proc Natl Acad Sci U S A, 2006
Oka T.
europepmc   +1 more source

Multiscale Perspectives on Solid-Phase Astrochemistry: Laboratory, Computation, and Open Questions. [PDF]

Space Sci Rev
Dickers MD, Mifsud DV, Mason NJ, Fantuzzi F.   +3 more
europepmc   +1 more source

Dissipative processes in galaxy formation. [PDF]

Proc Natl Acad Sci U S A, 1993
Silk J.
europepmc   +1 more source

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.
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SUZAKU OBSERVATIONS OF LOCAL ULTRALUMINOUS INFRARED GALAXIES

SUZAKU OBSERVATIONS OF LOCAL ULTRALUMINOUS INFRARED GALAXIES
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Ultraluminous Infrared Galaxies at 1.5

2007
We present measurements of the spatial clustering of ultraluminous infrared galaxies in two redshift intervals, 1.51.
Farrah, D., Lonsdale, C. J., Borys, C., Fang, F., Waddington, I., Oliver, S., Rowan-Robinson, M., Babbedge, T., Shupe, D., Polletta, M., Smith, H. E., Surace, J.   +11 more
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Ultraluminous Infrared Galaxies: Far-Infrared Highlights

Astrophysics and Space Science, 1999
We discuss two significant recent developments in the far-IRwith relevance to the study of Ultraluminous Infrared Galaxies(ULIRGs). The first of these is the discovery of an isotropiccosmological infrared background radiation (CIB). This has beendetected in observations by two different instruments (FIRAS (Puget etal. 1996, Hauser et al.
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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
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Ejection from Ultraluminous Infrared Galaxies

2000
Active galaxies, particularly Seyferts, have been shown to eject material in various forms including quasars with high intrinsic redshifts. A class of active galaxy which has so far not been analyzed from this standpoint is the so called Ultra Luminous Infrared Galaxies (ULRIG’s).
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Near-Infrared Spectroscopy of Ultraluminous Infrared Galaxies

1994
We report K band spectra of fourteen ultraluminous (LIR ≥ 1012L⊙) galaxies from the IRAS Extended Bright Galaxy Sample (EBGS) and ten less luminous EBGS galaxies. For the lower luminosity systems, good correlations are found between the H2 v=1-0S(1) and far-infrared (FIR) fluxes, and Brγ and FIR fluxes.
J. D. Goldader, R. D. Joseph, D. B. Sanders, R. Doyon   +3 more
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