Results 1 to 10 of about 3,101,923 (210)

The Evolution of the Star-Forming Interstellar Medium Across Cosmic Time [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2020
Over the past decade increasingly robust estimates of the dense molecular gas content in galaxy populations between redshift 0 and the peak of cosmic galaxy/star formation from redshift 1-3 have become available. This rapid progress has been possible due
L J Tacconi, R Genzel, Amiel Sternberg
exaly   +2 more sources

The cosmic evolution of magnesium isotopes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
The abundance of magnesium in the interstellar medium is a powerful probe of star formation processes over cosmological timescales. Magnesium has three stable isotopes, 24Mg, 25Mg, 26Mg, which can be produced both in massive and intermediate-mass (IM) stars with masses between 2 and 8 M_\odot.
Vangioni, E., Olive, K.A.
openaire   +4 more sources

Study of cosmic evolution admitting thermodynamic analysis [PDF]

open access: yesEuropean Physical Journal C: Particles and Fields
This article examines the cosmic evolution in the framework of symmetric teleparallel theory, characterized by the function of non-metricity scalar $$(\mathcal {Q})$$ ( Q ) .
M. Sharif, M. Zeeshan Gul, Nusrat Fatima
doaj   +2 more sources

Cosmic evolution of radio-AGN feedback: confronting models with data [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
Radio-mode feedback is a key ingredient in galaxy formation and evolution models, required to reproduce the observed properties of massive galaxies in the local Universe.
R. Kondapally   +13 more
semanticscholar   +1 more source

Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2022
We present the first model-agnostic analysis of the complete set of Sloan Digital Sky Survey III (BOSS) and -IV (eBOSS) catalogues of luminous red galaxy and quasar clustering in the redshift range 0.2 ≤ z ≤ 2.2 (10 billion years of cosmic evolution ...
S. Brieden, H. Gil-Marín, L. Verde
semanticscholar   +1 more source

Impact of massive binary star and cosmic evolution on gravitational wave observations II: Double compact object rates and properties [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2021
Making the most of the rapidly increasing population of gravitational-wave detections of BH and NS mergers requires comparing observations with population synthesis predictions. In this work we investigate the combined impact from the key uncertainties
F. Broekgaarden   +11 more
semanticscholar   +1 more source

Cosmic Evolution of the Logarithmic f(R) Model and the dS Swampland Conjecture [PDF]

open access: yesUniverse, 2021
In this paper, we study the inflationary scenario in logarithmic f(R) gravity, where the rate of inflation roll is constant. On the other hand, our gravitational f(R) model is a polynomial plus a logarithmic term.
J. Sadeghi   +4 more
semanticscholar   +1 more source

Cosmic Evolution of Barred Galaxies up to z ∼ 0.84 [PDF]

open access: yesAstrophysical Journal, 2021
We explore the cosmic evolution of the bar length, strength, and light deficit around the bar for 379 barred galaxies at 0.2 < z ≤ 0.835 using F814W images from the COSMOS survey.
Taehyun Kim   +6 more
semanticscholar   +1 more source

The Cosmic Evolution of Binary Black Holes in Young, Globular and Nuclear Star Clusters: Rates, Masses, Spins and Mixing Fractions [PDF]

open access: yes, 2021
The growing population of binary black holes (BBHs) observed by gravitational wave detectors is a potential Rosetta stone for understanding their formation channels. Here, we use an upgraded version of our semi-analytic codes fastcluster and cosmoRate to
M. Mapelli   +4 more
semanticscholar   +1 more source

Evolution of cosmic filaments in the MTNG simulation [PDF]

open access: yesAstronomy & Astrophysics, 2023
We present a study of the evolution of cosmic filaments across redshift with an emphasis on some important properties: filament lengths, growth rates, and radial profiles of galaxy densities.
Daniela Gal'arraga-Espinosa   +13 more
semanticscholar   +1 more source

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