Results 51 to 60 of about 216,275 (179)

Breathing FIRE: How Stellar Feedback Drives Radial Migration, Rapid Size Fluctuations, and Population Gradients in Low-Mass Galaxies [PDF]

open access: yes, 2016
We examine the effects of stellar feedback and bursty star formation on low-mass galaxies ($M_{\rm star}=2\times10^6-5\times10^{10}{\rm M_{\odot}}$) using the FIRE (Feedback in Realistic Environments) simulations.
Chan, T. K.   +6 more
core   +3 more sources

Feedback and the formation of dwarf galaxy stellar haloes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2009
Stellar population studies show that low mass galaxies in all environments exhibit stellar halos that are older and more spherically distributed than the main body of the galaxy. In some cases, there is a significant intermediate age component that extends beyond the young disk. We examine a suite of Smoothed Particle Hydrodynamic (SPH) simulations and
J. Wadsley   +6 more
openaire   +3 more sources

M-σ relations across cosmic time

open access: yesThe Open Journal of Astrophysics, 2023
Feedback from active galactic nuclei (AGN) has long been invoked to explain the correlation between black hole mass and stellar velocity dispersion (M-σ) discovered in low redshift galaxies. We describe the time evolution of AGN in the M-σ plane based on
David Garofalo   +5 more
doaj   +1 more source

Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation [PDF]

open access: yesMNRAS, 445, 581 (2014), 2013
We present a series of high-resolution cosmological simulations of galaxy formation to z=0, spanning halo masses ~10^8-10^13 M_sun, and stellar masses ~10^4-10^11. Our simulations include fully explicit treatment of both the multi-phase ISM (molecular through hot) and stellar feedback.
arxiv   +1 more source

Shaken or Stirred: The Diffuse Interstellar Medium with Exceptionally High SiO Abundance

open access: yesThe Astrophysical Journal, 2023
Interstellar shocks, a key element of stellar feedback processes, shape the structure of the interstellar medium (ISM) and are essential for the chemistry, thermodynamics, and kinematics of interstellar gas.
Daniel R. Rybarczyk   +2 more
doaj   +1 more source

Black Holes on FIRE: Stellar Feedback Limits Early Feeding of Galactic Nuclei [PDF]

open access: yes, 2017
We introduce massive black holes (BHs) in the Feedback In Realistic Environments project and perform high-resolution cosmological hydrodynamic simulations of quasar-mass halos ($M_{\rm halo}(z=2) \approx 10^{12.5}\,\rm{M}_{\odot}$) down to $z=1$.
Anglés-Alcázar, Daniel   +7 more
core   +3 more sources

Star Formation Variability as a Probe for the Baryon Cycle within Galaxies

open access: yesThe Astrophysical Journal, 2023
We investigate the connection between the regulation of star formation and the cycling of baryons both within and in and out of galaxies. We use idealized numerical simulations of Milky Way–mass galaxies, in which we vary the galaxy morphology and ...
Eun-jin Shin   +4 more
doaj   +1 more source

Stellar feedback in galaxies and the origin of galaxy-scale winds [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2012
16 pages, 11 figures, accepted to MNRAS (matches accepted version).
Hopkins, Philip F.   +2 more
openaire   +6 more sources

PHANGS–JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628

open access: yesThe Astrophysical Journal Letters, 2023
We present a high-resolution view of bubbles within the Phantom Galaxy (NGC 628), a nearby (∼10 Mpc), star-forming (∼2 M _⊙ yr ^−1 ), face-on ( i ∼ 9°) grand-design spiral galaxy.
Ashley. T. Barnes   +53 more
doaj   +1 more source

Stellar Feedback Up And Close

open access: yes, 2017
We report the serendipitous discovery of ongoing stellar feedback in the star-bursting nuclear ring of a nearby spiral galaxy, as part of the TIMER survey with MUSE. Combining MUSE and ALMA data we show bubbles of ionised gas expanding from the ring and shocking with the cold ISM.
Dimitri A. Gadotti, Timer Team
openaire   +2 more sources

Home - About - Disclaimer - Privacy