Results 191 to 200 of about 833,890 (231)
How the James Webb Space Telescope Is Revealing the Weather and Chemistry on Planets around Other Stars. [PDF]
Extance A.
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A follow-up strategy enabling discovery of electromagnetic counterparts to highly magnified gravitationally lensed gravitational waves. [PDF]
Ryczanowski D +8 more
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Strong long-term variability in active galactic nuclei affects virial black hole mass measurements. [PDF]
Amrutha N +7 more
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Extended hot dust emission around the earliest massive quiescent galaxy
Ji Z +16 more
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Hyperluminous infrared galaxies [PDF]
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 Galaxies in Compact Groups
Astrophysics and Space Science, 2003IR properties of Compact Group (CG) galaxies are presented and compared with IR properties of isolated galaxies. Despite CGs displaying more E-SOs and optically bright galaxies, no differences are retrieved concerning FIR emission. The observed lack of strong FIR enhancement in the CG sample is not surprising when interpreting FIR sources in CGs as ...
B. Kelm, P. Focardi, A. Zampieri
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BLAST: the far-infrared/radio correlation in distant galaxies [PDF]
We investigate the correlation between far-infrared (FIR) and radio luminosities in distant galaxies, a lynchpin of modern astronomy. We use data from the Balloon-borne Large Aperture Submillimetre Telescope (BLAST), Spitzer, the Large Apex BOlometer ...
Rob Ivison, Attila Kovacs, Simon Dye
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An infrared search for primeval galaxies
1994We present early results of a near-infrared search for Primeval Galaxies (PGs), i.e., galaxies forming the bulk of their stars at high redshift. These results are compared with some theoretical expectations on the surface density of the PGs.
F. Mannucci +2 more
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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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