Results 191 to 200 of about 36,025 (222)
A detailed analysis of the Czernik 38 cluster and its associated tidal tail, utilizing Gaia DR3 and 2MASS. [PDF]
Ahmed NM.
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Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn
Fujimoto S +45 more
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A Network Approach for the Accurate Characterization of Water Lines Observable in Astronomical Masers and Extragalactic Environments. [PDF]
Ubachs W +4 more
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Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]
Di Mascolo L +25 more
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Infrared bands of neutral gas-phase carbon clusters in a broad spectral range.
Ferrari P, Lemmens AK, Redlich B.
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Spectroscopic confirmation of two luminous galaxies at a redshift of 14 [PDF]
Christopher N A Willmer +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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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
2008There has been considerable recent interest in the properties of infrared galaxies due to the discovery by the Infrared Astronomical Satellite (IRAS) of a class of luminous galaxies which emit the bulk of their energy in the far-infrared (Houck et al. 1984; Soifer et al. 1984).
Sanders, D. B. +2 more
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