Results 101 to 110 of about 144,375 (218)
Post-starburst galaxies and the transformation of blue into red galaxies [PDF]
We present deep single-dish radio observations of a sample of nearby post-starburst galaxies (0.05 < z < 0.1). About 50% of these post-starburst galaxies are detected at 21 cm, with H I masses of ~109M⊙, up to ~1010M⊙.
Pisano, Daniel +4 more
core +1 more source
38 pages including 4 tables, 7 postscript figures. To appear in ApJS, December 1998 Vol.
Coziol, R. +4 more
openaire +2 more sources
The properties of discrete X-ray sources in star-forming galaxies [PDF]
Observations of starburst galaxies have revealed a large number of point-like X-ray sources located within these systems, including active galactic nuclei (AGN), X-ray binaries (XRBs), and utraluminous X-ray sources (ULXs).
JACKSON, FLOYD,EMMANUEL
core
Early assembly of the most massive galaxies [PDF]
The current consensus is that galaxies begin as small density fluctuations in the early Universe and grow by in situ star formation and hierarchical merging(1).
Chris A. Collins +53 more
core +1 more source
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
doaj +1 more source
Polarized thermal emission from dust in a galaxy at redshift 2.6. [PDF]
Geach JE +7 more
europepmc +1 more source
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
doaj +1 more source
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 ...
openaire +1 more source
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
doaj +1 more source
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.
openaire +2 more sources

