Results 61 to 70 of about 216,275 (179)
The IMF of stellar clusters: effects of accretion and feedback [PDF]
Monthly Notices of the Royal Astronomical Society, 2010 accepted to MNRAS. 22 pages, 17 figures. 2 new sections added to better present the model parameters and compare to previous work. Some figures are now better presented.
G. Maheswar +5 more
openaire +3 more sources
The energy and dynamics of trapped radiative feedback with stellar winds
Monthly Notices of the Royal Astronomical Society, 2023 ABSTRACT In this paper, we explore the significant, non-linear impact that stellar winds have on H ii regions. We perform a parameter study using three-dimensional radiative magnetohydrodynamic simulations of wind and ultraviolet radiation feedback from a 35 M⊙ star formed self-consistently in a turbulent, self-gravitating cloud, similar
Geen, Sam +4 more
openaire +7 more sources
Stellar Feedback and Resolved Stellar IFU Spectroscopy in the Nearby Spiral Galaxy NGC 300 [PDF]
The Astrophysical Journal, 2020 Abstract We present MUSE integral field unit (IFU) observations of five individual H ii regions in two giant star-forming complexes in the low-metallicity, nearby dwarf spiral galaxy NGC 300. In combination with high spatial resolution Hubble Space Telescope photometry, we demonstrate the extraction of stellar spectra and classification ...
Nell Byler +12 more
openaire +3 more sources
Modeling for Stellar Feedback in Galaxy Formation Simulations [PDF]
The Astrophysical Journal, 2017 Abstract Various heuristic approaches to model unresolved supernova (SN) feedback in galaxy formation simulations exist to reproduce the formation of spiral galaxies and the overall inefficient conversion of gas into stars. Some models, however, require resolution-dependent scalings.
Jeremiah P. Ostriker +6 more
openaire +4 more sources
Formation of Massive and Wide First-star Binaries in Radiation Hydrodynamic Simulations
The Astrophysical Journal, 2023 We study the formation of Population III stars by performing radiation hydrodynamic simulations for three different initial clouds extracted from cosmological hydrodynamic simulations.
Kazuyuki Sugimura +4 more
doaj +1 more source
Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback [PDF]
, 2021 A recent comparison by Merritt et al. 2020 of simulated and observed Milky Way-mass galaxies has identified a significant tension between the outskirts ($r>20\kpc$) of the stellar halos in simulated and observed galaxies. Using observations from the Dragonfly telescope and simulated galaxies from the Illustris-TNG100 project, Merritt et al.
arxiv +1 more source
A Systematic Look at the Effects of Radiative Feedback on Disc Galaxy Formation [PDF]
, 2014 Galaxy formation models and simulations rely on various feedback mechanisms to reproduce the observed baryonic scaling relations and galaxy morphologies. Although dwarf galaxy and giant elliptical properties can be explained using feedback from supernova
Agertz, Oscar +4 more
core +1 more source
The origin of ultra diffuse galaxies: stellar feedback and quenching [PDF]
Monthly Notices of the Royal Astronomical Society, 2018 20 pages, 13 figures; match the MNRAS accepted ...
Claude André Faucher-Giguère +9 more
openaire +7 more sources
Observational constraints on stellar feedback in dwarf galaxies
Nature Astronomy, 2022 Invited Perspective article, accepted for publication in Nature ...
Michelle L. M. Collins, Justin I. Read
openaire +2 more sources
Frontiers in Astronomy and Space Sciences, 2017 We present the galactic stellar age—velocity dispersion relation obtained from a semi-analytic model of galaxy formation. We divide galaxies into two populations: galaxies which have over-massive/under-massive black holes (BHs) against the best-fitting ...
Hikari Shirakata +3 more
doaj +1 more source