Results 201 to 210 of about 2,538 (226)
Adaptive Optics Discovery of Supernova 2004ip in the Nuclear Regions of the Luminous Infrared Galaxy IRAS 18293-3413 [PDF]
Astrophysical Journal, 2007 Publicación ISIWe report a supernova discovery in K-s-band images from the NAOS CONICA adaptive optics (AO) system on the ESO Very Large Telescope. The images were obtained as part of a near- infrared search for highly obscured supernovae in the nuclear ...
, Andreas Efstathiou, T Dahlen
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Annual Review of Astronomy and Astrophysics, 1996
▪ Abstract At luminosities above 1011 [Formula: see text], infrared galaxies become the dominant population of extragalactic objects in the local Universe (z ≲ 0.3), being more numerous than optically selected starburst and Seyfert galaxies and quasi-stellar objects at comparable bolometric luminosity.
D. B. Sanders, I. F. Mirabel
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▪ Abstract At luminosities above 1011 [Formula: see text], infrared galaxies become the dominant population of extragalactic objects in the local Universe (z ≲ 0.3), being more numerous than optically selected starburst and Seyfert galaxies and quasi-stellar objects at comparable bolometric luminosity.
D. B. Sanders, I. F. Mirabel
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DISCOVERY OF TWO SUPERNOVAE IN THE NUCLEAR REGIONS OF THE LUMINOUS INFRARED GALAXY IC 883 [PDF]
Astrophysical Journal Letters, 2012 6 páginas, 3 figuras, 1 tabla.-- Kankare, E. et al.We report the discovery of two consecutive supernovae (SNe), 2010cu and 2011hi, located at 0.37" (180 pc) and 0.79" (380 pc) projected distance respectively from the centre of the K-band nucleus of the ...
, Erkki Kankare, Andreas Efstathiou
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Hubble Ultra Deep Field–JD2: Mid‐Infrared Evidence for a z∼ 2 Luminous Infrared Galaxy [PDF]
Astrophysical Journal, 2007 The Hubble Ultra Deep Field source JD2 presented in Mobasher et al. is an unusual galaxy that is very faint at all wavelengths shortward of 1.1 μm. Photometric redshift fits to data between 0.4 and 8 μm yield a significant probability that it is an ...
Casey Papovich
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AEGIS: Infrared Spectroscopy of an Infrared-luminous Lyman Break Galaxy at z = 3.01 [PDF]
Astrophysical Journal, 2007 We report the detection of rest-frame 6.2 and 7.7 μm emission features arising from polycyclic aromatic hydrocarbons (PAHs) in the Spitzer IRS spectrum of an infrared-luminous Lyman break galaxy at z = 3.01.
Rob Ivison, Pauline Barmby
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Chandraobservations of the luminous infrared galaxy NGC 3256 [PDF]
Monthly Notices of the Royal Astronomical Society, 2002 Artículo de publicación ISIWe present a detailed analysis of high-resolution Chandra observations of the merger system NGC 3256, the most infrared-luminous galaxy in the nearby universe.
Almudena Alonso-Herrero +2 more
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The AGN/starburst connection in luminous infrared galaxies
Advances in Space Research, 1999Abstract One of the most exciting results of the IRAS sky survey was the discovery of luminous infrared galaxies, which emit the bulk of their radiataion in the infrared. One of the most vexing questions about luminous infrared galaxies is the relative contribution of starburst or AGN to the overall energy budget.
L.J. Kewley +3 more
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CO in infrared luminous galaxies
2008© 1988 Springer-Verlag.
Sanders, D. B. +2 more
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The Environments of Luminous Infrared Galaxies
2011This work studies the relationship between SFR, stellar mass and environment of local IR galaxies, especially LIRGs. It is found that the L { IR} ∼ 1011 L ⊙ marks an important luminosity point among IR galaxies - the large scale density of environment around LIRGs correlates strongly with their SFR above this value at a fixed stellar mass. On the other
A. G. Tekola, P. Väisänen, A. Berlind
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ISO spectroscopy of luminous infrared galaxies
Advances in Space Research, 2000Abstract Spectroscopy from the Infrared Space Observatory ISO has for the first time provided the sensitivity to observe mid-infrared fine structure lines and PAH features in a wide range of luminous infrared galaxies. We report on observations obtained with SWS, ISOPHOT-S, and the ISOCAM CVF and show that the mid-IR spectral features are excellent ...
R. Genzel, D. Lutz
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