召集
发表于 2025-3-28 16:48:54
Gas Accretion and Star Formation Rates,l metallicity relationship, the relationship between disk morphology and gas metallicity, the existence of metallicity drops in starbursts of star-forming galaxies, the so-called G dwarf problem, the existence of a minimum metallicity for the star-forming gas in the local universe, the origin of the
AWRY
发表于 2025-3-28 18:58:04
Gas Accretion Traced in Absorption in Galaxy Spectroscopy,e II has provided evidence for ongoing gas accretion onto > 5% of luminous, star-forming galaxies at . ∼ 0. 5–1. We then discuss the potentially ground-breaking benefits of future efforts to improve the spectral resolution of such studies, and to leverage spatially resolved spectroscopy for new cons
Indicative
发表于 2025-3-29 00:17:16
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外来
发表于 2025-3-29 04:55:22
The Circumgalactic Medium in Massive Halos,m massive quiescent galaxies. The origin of the gas closer in is currently less certain, but SNe Ia driven winds appear to contribute significantly to cool gas found at . < 100 kpc. In contrast, cool gas observed at . kpc from luminous quasars appears to be intimately connected to quasar activities
柔声地说
发表于 2025-3-29 07:28:34
Gas Accretion and Giant Ly, Nebulae,f massive galaxies. Spectroscopic studies suggest that, among the giant Ly. nebulae, the one associated with radio-loud AGN should have kinematics dominated by strong, ionized outflows within at least the inner 30–50 kpc. Radio-quiet nebulae instead present more quiescent kinematics compatible with
蔓藤图饰
发表于 2025-3-29 14:57:23
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人工制品
发表于 2025-3-29 18:11:14
Gas Accretion and Angular Momentum,to the central galaxy. We discuss the implications of these simulations, reviewing a number of recent developments in the literature, and suggest a revision to the canonical model as it relates to the expected angular momentum content of gaseous halos around galaxies.
举止粗野的人
发表于 2025-3-29 20:52:15
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AND
发表于 2025-3-30 00:16:07
0067-0057 retion is a rare area of astrophysics in which the basic theoretical predictions are established, but the observations have been as yet unable to verify the expectations. Accretion has long been seen around the978-3-319-84920-1978-3-319-52512-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
自传
发表于 2025-3-30 04:33:17
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