Results 121 to 130 of about 146,314 (245)
Different Influence of Gas Accretion on the Evolution of Star-forming and Non-star-forming Galaxies
Using integral field spectroscopic data from the Mapping Nearby Galaxies at Apache Point Observatory survey, we investigate the spatially resolved properties and empirical relations of a star-forming galaxy and a non-star-forming galaxy hosting ...
Min Bao, Wenlong Zhao, Qirong Yuan
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Starburst Galaxies in Their Last Billion Years: An Hδ Absorption Line Selected Sample
In this paper, we focus on the study of starburst galaxies in their final billion years. Our galaxy selection is based solely on the presence of the H δ absorption line, which permits the later evolution of starburst galaxies to be traced, coinciding ...
Shumei Wu +3 more
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Spin statistics in binary galaxies - Implications for formation and evolution
G. Hélou
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Secular evolution of late-type disc galaxies: formation of bulges and the origin of bar dichotomy [PDF]
Masafumi Noguchi
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We have used public JWST/NIRSpec and JWST/NIRCam observations from the CEERS and JADES surveys in order to analyze the star-forming main sequence (SFMS) over the redshift range 1.4 ≤ z < 7.
Leonardo Clarke +7 more
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Galaxy formation and evolution -- II. Energy balance, star formation and feedback [PDF]
F. Buonomo +3 more
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Analysis of Galaxies at the Extremes: Failed Galaxy Progenitors in the MAGNETICUM Simulations
There is increasing observational evidence for a “failed galaxy” formation pathway for ultra-diffuse galaxies (UDGs) at low redshift however they currently lack simulated counterparts.
Jonah S. Gannon +7 more
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The formation of the Hubble sequence of disc galaxies: the effects of early viscous evolution [PDF]
Bing Zhang, Rosemary F. Ġ. Wyse
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Star Formation and Dust in the Cosmic Web
The large-scale environment of the cosmic web is believed to impact galaxy evolution, but there is still no consensus regarding the mechanisms. We use a semi-analytic model (SAM) galaxy catalog to study the star formation and dust content of local ...
Massimiliano Parente +10 more
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We explore the effect of variations in the Population III initial mass function (IMF) and star-by-star feedback on early galaxy formation and evolution using the A eos simulations. We compare simulations with two different Population III IMFs: M _char =
Kaley Brauer +9 more
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