Results 81 to 90 of about 683 (187)
Energetic Particles in Clusters of Galaxies and Starburst Galaxies
14 pages, 5 figures: Invited paper presented at "The Universe Viewed in Gamma-Rays" held on 25-28 Sept. 2002 in Kashiwa Japan.
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The Galactic Centre - a laboratory for starburst galaxies (?) [PDF]
AbstractThe Galactic centre – as the closest galactic nucleus – holds both intrinsic interest and possibly represents a useful analogue to starburst nuclei which we can observe with orders of magnitude finer detail than these external systems. The environmental conditions in the GC – here taken to mean the inner 200 pc in diameter of the Milky Way ...
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We present the number densities and physical properties of the bright galaxies spectroscopically confirmed at z ∼ 7–14. Our sample is composed of 60 galaxies at z _spec ∼ 7–14, including recently confirmed galaxies at z _spec = 12.34–14.18 with JWST, as ...
Yuichi Harikane +35 more
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Polarized thermal emission from dust in a galaxy at redshift 2.6. [PDF]
Geach JE +7 more
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New multiaperture 1.65 and 2.2 micron photometry has been obtained for the central region of 132 spirals exhibiting 2 orders of magnitude range in central 10-micron luminosity. This multiaperture photometry along with optical spectroscopy indicated that the high central 10-micron luminosity (about 1 billion solar luminosities) is powered by massive ...
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38 pages including 4 tables, 7 postscript figures. To appear in ApJS, December 1998 Vol.
Coziol, R. +4 more
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Caught in the Act of Quenching? -- A Population of Post-Starburst Ultra-Diffuse Galaxies
We report the discovery of post-starburst ultra-diffuse galaxies (UDGs), identified through spectroscopic analysis with KCWI at the Keck II Telescope. Our analysis is based on a sample of 44 candidate UDGs selected from the Systematically Measuring Ultra-
Loraine Sandoval Ascencio +5 more
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We present detailed spectral energy distribution (SED) modeling of 14 local ultraluminous infrared galaxies (ULIRGs) with outstanding photometric data from the literature covering the ultraviolet–infrared (FIR) and radio bands (∼50 MHz to ∼30 GHz).
Subhrata Dey +3 more
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Infrared-luminous galaxies are important sites of stellar and black hole mass assembly at most redshifts. Their luminosities are often estimated by fitting spectral energy distribution (SED) models to near- to far-infrared data, but the dependence of ...
Duncan Farrah +25 more
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The Evolution of Starburst Galaxies
8 pages, 4 figures, to be published in proceedings of the MPIA workshop, "Modes of Star Formation and the Origin of Field Star Populations", ed. E.
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