Results 141 to 150 of about 689 (170)

Active galactic nuclei. [PDF]

Proc Natl Acad Sci U S A, 1999
Fabian AC.
europepmc   +1 more source

Accurate determination of chemical abundances near a supermassive black hole. [PDF]

Nat Astron
XRISM Collaboration.
europepmc   +1 more source

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.
openaire  

Extinction law in ultraluminous infrared galaxies at z∼ 1 [PDF]

Monthly Notices of the Royal Astronomical Society, 2011
We analyse the multiwavelength photometric and spectroscopic data of 12 ultraluminous infrared galaxies (ULIRGs) at z∼1 and compare them with models of stars and dust in order to study the extinction law and star formation in young infrared (IR) galaxies.
K Kawara, N Ienaka, T Kozasa
exaly   +2 more sources

Some of the next articles are maybe not open access.

Related searches:

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, Shchekinov Yu A   +2 more
exaly   +2 more sources

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).
openaire   +2 more sources

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
openaire   +1 more source