Results 81 to 90 of about 1,645,813 (249)

Cis–Trans Rotational Isomerism of Formic Acid, Sulfur, and Selenium Analogues and Their Dimers: Chemical Kinetics Under Interstellar Conditions

open access: yesInternational Journal of Chemical Kinetics, EarlyView.
ABSTRACT We present chemical kinetic rate constants for the cis to trans isomerisation or rotamerization of monomeric seleno‐, thio‐, and formic acids and that of three of their dimeric species, based on variational transition state theory and multidimensional tunneling calculations in the gas‐phase, from 10 K to 300 K. These provide, firstly, reliable
Judith Wurmel, John M. Simmie
wiley   +1 more source

The AGORA High-resolution Galaxy Simulations Comparison Project. X. Formation and Evolution of Galaxies at the High-redshift Frontier

open access: yesThe Astrophysical Journal
Recent observations from the James Webb Space Telescope have revealed unexpectedly luminous galaxies, exhibiting stellar masses and luminosities significantly higher than predicted by theoretical models at Cosmic Dawn.
Hyeonyong Kim   +25 more
doaj   +1 more source

Identification of clusters of galaxies and physical properties of clusters and their member galaxies [PDF]

open access: yesChinese Science Bulletin, 2019
Clusters of galaxies are the largest gravitationally bound systems in the Universe and are located at the knots of cosmic web. They provide powerful constraints on galaxy evolution, the formation of large scale structure of the Universe and many astrophysical processes.
Jinlin Han   +3 more
openaire   +1 more source

Introducing the DREAMS Project: DaRk mattEr and Astrophysics with Machine Learning and Simulations

open access: yesThe Astrophysical Journal
We introduce the DaRk mattEr and Astrophysics with Machine learning and Simulations (DREAMS) project, an innovative approach to understanding the astrophysical implications of alternative dark matter (DM) models and their effects on galaxy formation and ...
Jonah C. Rose   +29 more
doaj   +1 more source

Galaxy formation and physical bias

open access: yesThe Astrophysical Journal, 1992
We have supplemented our code, which computes the evolution of the physical state of a representative piece of the universe to include, not only the dynamics of dark matter (with a standard PM code), and the hydrodynamics of the gaseous component (including detailed collisional and radiative processes), but also galaxy formation on a heuristic but ...
Renyue Cen, Jeremiah P. Ostriker
openaire   +1 more source

The physical properties of Lyαemitting galaxies: not just primeval galaxies? [PDF]

open access: yesAstronomy & Astrophysics, 2008
Accepted by Astronomy & ...
Pentericci, L.   +6 more
openaire   +2 more sources

Simulating molecular cloud regulated star formation in Galaxies [PDF]

open access: yes, 2007
This thesis is primarily concerned with understanding the process of galaxy formation via the simulation of the interstellar medium, star formation and supernova feedback.
Booth, Craig Martin
core  

Human Sustainability Leadership and Employee Wellbeing (Flourishing) in Organizations

open access: yesSustainable Development, EarlyView.
ABSTRACT This qualitative case study research examines how designing for human sustainability leadership (HSL) affects employee wellbeing (flourishing) (HWBF) in organizations. It is undertaken at a university in the United Kingdom including academics and administrators.
Elli Meleti
wiley   +1 more source

A Splashback-like Feature of Central Galaxies in Galaxy Clusters

open access: yesThe Astrophysical Journal
We investigate a splashback-like feature in the outer region of central galaxies (CGs) in clusters. This feature is detected as a “dip” in the radial slope of the CG surface brightness, derived through the stacking of Dark Energy Survey data of over 4000
Yuanyuan Zhang   +5 more
doaj   +1 more source

The Physics of Galaxy Accretion

open access: yes
How do galaxies get the gas needed to fuel star formation?' remains a fundamental open question, even for the Milky-Way. I will review recent theoretical developments in galaxy accretion physics, which go beyond the classic separation between 'cold' and 'hot' accretion. I will also discuss the potential implications of different accretion modes for the
Stern, Jonathan   +8 more
openaire   +1 more source

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