Results 11 to 20 of about 14,291 (188)
The nature of hyperluminous infrared galaxies [PDF]
Astronomy & Astrophysics, 2021 Context. Hyperluminous infrared galaxies (HLIRGs) are shown to have been more abundant in early epochs. The small samples used in earlier studies are not sufficient to draw robust statistical conclusions regarding the physical properties and the power sources of these extreme infrared (IR) bright galaxies. Aims.
Gao, F. +9 more
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Modeling the evolution of infrared galaxies: clustering of galaxies in the cosmic infrared background [PDF]
Astronomy & Astrophysics, 2012 Star-forming galaxies are a highly biased tracer of the underlying dark matter density field. Their clustering can be studied through the cosmic infrared background anisotropies. These anisotropies have been measured from 100 \mum to 2 mm in the last few years. In this paper, we present a fully parametric model allowing a joint analysis of these recent
Pénin, A. +3 more
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The infrared luminosity of galaxy clusters [PDF]
Astronomy & Astrophysics, 2008 9 pages, 7 figures, accepted july 31st 2008 for publication in Astronomy and Astrophysics, language improved for this ...
Giard, M. +3 more
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Near-Infrared Spectra of Ultraluminous Infrared Galaxies [PDF]
The Astrophysical Journal, 1999 Near infrared spectra with resolution R ~ 1100 in the rest wavelength range 1.8-2.2 microns have been obtained for a complete sample of 33 ultraluminous infrared galaxies. Of the 33 objects observed, 2 show evidence of a central AGN through either a broad Paschen-alpha line or emission in the 1.963 micron fine structure of [Si VI].
Murphy, Jr., T. W. +4 more
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Mid infrared polarisation of Ultraluminous Infrared Galaxies [PDF]
Astronomy & Astrophysics, 2001 The mid infrared polarisation properties of four Ultraluminous Infrared Galaxies (ULIRGs) have been investigated by broad band filter observations with the ISOCAM instrument on board the Infrared Space Observatory (ISO). The wavelength region from 5 to 18 mic. was selected where the emission from the putative torus peaks.
Siebenmorgen, R., Efstathiou, A.
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Hyperluminous infrared galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2000 39 galaxies are now known, from follow-up of faint IRAS sources and from submm observations of high redshift AGN, with far infrared luminosities > 10^{13} Lo. 13 of these, which have been found in 60 or 850 mu surveys, form an important unbiased sub-sample.
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Infrared polarimetry of galaxies. I - Infrared luminous galaxies
The Astrophysical Journal, 1989 Les observations polarimetriques a 1.2, 1.65 et 2.2 μm sont presentees pour les noyaux de 6 galaxies IR lumineuses: IRAS 05189-2524, UGC 5101, Mrk 231, Mrk 273, Arp 220 et NGC 6240. Les nombreux mecanismes et les geometries responsables de la production de la polarisation dans le proche IR sont discutes en ...
Terry Jay Jones, Dimitri Klebe
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MID-INFRARED SPECTRAL DIAGNOSTICS OF LUMINOUS INFRARED GALAXIES [PDF]
The Astrophysical Journal, 2011 accepted for publication in ApJ, 34 pages, 12 ...
Petric, A. O. +24 more
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Ultraluminous Infrared Galaxies: Atlas of Near‐Infrared Images [PDF]
The Astrophysical Journal Supplement Series, 2002 To appear in ApJSupp; 9 embedded figures; Complete ps copy with higher resolution figures available at http://www.stsci.edu ...
Bushouse, H A +8 more
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Far‐Infrared Galaxies in the Far‐Ultraviolet [PDF]
The Astrophysical Journal, 2002 In an effort to better understand the UV properties of ultraluminous infrared galaxies (ULIGs), and compare them to the rest-frame UV properties of high redshift sub-mm and Lyman-break galaxies, we have obtained far- and near-UV imaging observations (lambda_{eff}=1457Å, lambda_{eff}=2364Å, respectively) of two luminous infrared galaxies (LIGs--VV 114 ...
Goldader, J. +6 more
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