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How do galaxies such as our Milky Way come into existence? How do they grow and change over time? The science behind galaxy formation has long been a puzzle, but a University of Arizona-led team of sc...
We present robust statistical estimates of the accuracy of early-type galaxy stellar masses derived from spectral energy distribution (SED) fitting as functions of various empirical and theoretical as...
We study the Kennicutt-Schmidt star formation law and efficiency in the gaseous disk of the isolated galaxy CIG 96 (NGC 864), with special emphasis on its unusually large atomic gas (HI) disk (r_HI/r_...
We analyze the dependence of galaxy structure (size and Sersic index) and mode of star formation (\Sigma_SFR and SFR_IR/SFR_UV) on the position of galaxies in the SFR versus Mass diagram. Our sample c...
Nuclear to host galaxy relation of high redshift quasars。
Big game hunting in the andromeda galaxy:identifying And weighing black holes in low mass x-ray binaries。
An x-ray view of interacting binaries outside the galaxy
The detection of supergalactic winds:The edge-on starburst galaxy NGC 4631。
N-Body Simulations of Small Galaxy Groups (Parte A)。
Iso spectroscopy of ultracompact H II regions:element abundance gradient in the galaxy
In this work, based on the analytical model with delayed production approximation developed by Pagel & Tautvaiˇsien˙e (1995) for the Galaxy, the analytic solutions of the distribution of neutron e...

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