Results 141 to 150 of about 216,275 (179)
The Dual Nature Of (Stellar) Feedback In Galaxy Evolution
, 2017 Feedback processes are central to the evolution of galaxies since they regulate the baryon flow to and from them. However, these processes are extremely difficult to simulate owing to large range of spatial scales that need to be modelled. In the cosmological context there is a general consensus on feedback being a “negative” process that limits the ...
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Intense Star Cluster Formation: Stellar Masses, the Mass Function, and the Fundamental Mass Scale
The Astrophysical Journal LettersWithin the birth environment of a massive globular cluster, the combination of a luminous young stellar population and a high column density induces a state in which the thermal optical depth and radiation pressure are both appreciable.
Christopher D. Matzner
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Kiloparsec-scale Simulations of Star Formation in Disk Galaxies. IV. Regulation of Galactic Star Formation Rates by Stellar Feedback [PDF]
, 2017 Michael J. Butler +5 more
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On the Signature of Black Holes on the Quenched Stellar Mass Function
The Astrophysical JournalAs star-forming galaxies approach or exceed a stellar mass of around 10 ^11 M _⊙ , they are increasingly likely to be quenched in a process generically called mass quenching.
Antonio J. Porras-Valverde +1 more
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Mechanical Feedback: From stellar wind bubbles to starbursts
, 2001 M. S. Oey, C. J. Clarke, Philip Massey
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Stellar Feedback and Chemical Evolution In Dwarf Galaxies
, 2019 Motivated by the desire to investigate two of the largest outstanding problems in galactic evolution -- stellar feedback and galactic chemical evolution -- we develop the first set of galaxy-scale simulations that simultaneously follow star formation with individual stars and their associated multi-channel stellar feedback and multi-element metal ...
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The Timescales of Star Cluster Emergence: The Case of NGC 4449
The Astrophysical JournalWe survey the young star cluster population in the dwarf galaxy NGC 4449 with the goal of investigating how stellar feedback may depend on the clusters’ properties.
Timothy McQuaid +9 more
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Magnetic Fields and Velocity Gradients in L1551: The Role of Stellar Feedback
, 2023 Mingrui Liu, Yue Hu, A. Lazarian
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