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Dissipative processes in galaxy formation. [PDF]
Proc Natl Acad Sci U S A, 1993 Silk J.
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HARMONI Observations of Luminous and Ultraluminous Infrared Galaxies
, 2015 Trabajo presentado en Early E-ELT Science: Spectroscopy with HARMONI, celebrado en el Oxford University Museum of History Natural (Oxford, Inglaterra), del 29 de junio al 3 de julio de ...
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Ultraluminous Infrared Galaxies: Far-Infrared Highlights [PDF]
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, 2017Ultraluminous 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 ...
E. O. Vasiliev +3 more
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Near-Infrared Spectroscopy of Ultraluminous Infrared Galaxies
1994We 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.
René Doyon +3 more
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Molecular Gas in Ultraluminous Infrared Galaxies
1997The discovery of CO emission (Wilson, Jefferts & Penzias 1970) 25 years ago opened a major new astronomical window which has led to important advances in many areas of Galactic and extragalactic astronomy. The strength and ubiquity of the CO lines, CO isotopic lines, and other millimeter transitions have provided extraordinary diagnostics for studying ...
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Ejection from Ultraluminous Infrared Galaxies
2000Active 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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InP colloidal quantum dots for visible and near-infrared photonics
Nature Reviews Materials, 2023Guilherme Almeida
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Ultraluminous Infrared Galaxies and Galaxy Formation
Astrophysics and Space Science, 1999openaire +2 more sources