Results 141 to 150 of about 2,636,463 (178)

What Drives the H i Content of Central Galaxies—A Comparison between Hydrodynamic Simulations and Observations Using Random Forest

open access: yesThe Astrophysical Journal
We investigate the driving mechanisms for the H i gas content in star-forming central galaxies at low redshift, by examining the H i -to-stellar mass ratio ( M _H _i / M _* ) in both the state-of-the-art hydrodynamic simulations, IllustrisTNG (TNG) and ...
Xiao Li, Cheng Li, H. J. Mo
doaj   +1 more source

The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation

open access: yesAstronomy & Astrophysics
We present the first results from the SMUGGLE-Ring project, a suite of simulations employing the Stars and MUltiphase Gas in GaLaxiEs (SMUGGLE) interstellar medium (ISM) and stellar feedback model to explore nuclear structures in Milky Way-mass galaxies.
Kwak SungWon   +10 more
doaj   +1 more source

Tracing the Origins of Hot Halo Gas in Milky Way–type Galaxies with SMUGGLE

open access: yesThe Astrophysical Journal
Current galaxy formation models predict the existence of X-ray-emitting gaseous halos around Milky Way (MW)–type galaxies. To investigate properties of this coronal gas in MW-like galaxies, we analyze a suite of high-resolution simulations based on the ...
Zhijie Zhang   +10 more
doaj   +1 more source

Stellar Population and Energy Feedback in the Supergiant Shell LMC 1

open access: yesThe Astronomical Journal
Supergiant shells (SGSs) are the largest interstellar structures in galaxies and inject hot enriched gas into galactic halos. We have studied SGS LMC 1 to determine quantitatively whether stellar energy feedback is adequate to power the formation of an ...
Guan-Hong Li   +6 more
doaj   +1 more source

Osaka Feedback Model. III. Cosmological Simulation CROCODILE

open access: yesThe Astrophysical Journal
We introduce our new cosmological simulation data set CROCODILE, executed using the GADGET4-Osaka smoothed particle hydrodynamics code. This simulation incorporates an updated supernova (SN) feedback model of Y. Oku et al.
Yuri Oku, Kentaro Nagamine
doaj   +1 more source

Correlation between Baryonic Process and Galaxy Assembly Bias

open access: yesThe Astrophysical Journal
Galaxy assembly bias (GAB) is the dependence of galaxy clustering on secondary properties beyond halo mass. In this work, we study the connections between GAB and baryonic processes using the Galacticus semianalytic model (SAM) for galaxy formation and ...
Zilan Xiao   +4 more
doaj   +1 more source

The stellar and dark matter distributions in early-type galaxies measured by stacked weak gravitational lensing

open access: yesThe Open Journal of Astrophysics
We investigate stellar mass and central dark matter density profiles of photometric luminous red galaxies with stellar masses of $\sim10^{10}-10^{12}M_\odot$ using weak gravitational lensing measurements from the Hyper Suprime-Cam Subaru Strategic ...
Momoka Fujikawa, Masamune Oguri
doaj   +1 more source

Stellar Feedback as Holographic Information Regulation

open access: yes
Application of Ontological Resolution Theory (ORT) to stellar astrophysics, demonstrating that stellar evolution is an active component of cosmological information regulation rather than merely a local thermodynamic process. Version 3 (November 2025) includes: • Rigorous effective horizon dynamics via screened Poisson equation on S² • Derivation of ...
openaire   +1 more source

Stellar Feedback and Chemical Evolution In Dwarf Galaxies

open access: yes, 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 ...
openaire   +2 more sources

Formation of the first galaxies under stellar feedback

open access: yes, 2015
The stellar feedback is a crucial ingredient for modeling galaxy formation, especially for the first galaxies, which are susceptible to stellar feedback due to their shallow potential wells.
Jeon, Myoungwon
core   +1 more source

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