The first stars: formation, properties, and impact
RS Klessen, SCO Glover - Annual Review of Astronomy and …, 2023 - annualreviews.org
The first generation of stars, often called Population III (or Pop III), form from metal-free
primordial gas at redshifts z∼ 30 and below. They dominate the cosmic star-formation …
primordial gas at redshifts z∼ 30 and below. They dominate the cosmic star-formation …
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical …
M Ruszkowski, C Pfrommer - The Astronomy and Astrophysics Review, 2023 - Springer
Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
Primordial black holes
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Journals & Books Search RegisterSign in View PDF Download full book Search ScienceDirect …
Journals & Books Search RegisterSign in View PDF Download full book Search ScienceDirect …
Mesa isochrones and stellar tracks (MIST). I. Solar-scaled models
J Choi, A Dotter, C Conroy, M Cantiello… - The Astrophysical …, 2016 - iopscience.iop.org
This is the first of a series of papers presenting the Modules for Experiments in Stellar
Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a new comprehensive …
Astrophysics (MESA) Isochrones and Stellar Tracks (MIST) project, a new comprehensive …
Models for the long-term variations of solar activity
BB Karak - Living Reviews in Solar Physics, 2023 - Springer
One obvious feature of the solar cycle is its variation from one cycle to another. In this article,
we review the dynamo models for the long-term variations of the solar cycle. By long-term …
we review the dynamo models for the long-term variations of the solar cycle. By long-term …
The origin, evolution and signatures of primordial magnetic fields
K Subramanian - Reports on Progress in Physics, 2016 - iopscience.iop.org
The universe is magnetized on all scales probed so far. On the largest scales, galaxies and
galaxy clusters host magnetic fields at the micro Gauss level coherent on scales up to ten …
galaxy clusters host magnetic fields at the micro Gauss level coherent on scales up to ten …
Magnetism, dynamo action and the solar-stellar connection
AS Brun, MK Browning - Living Reviews in Solar Physics, 2017 - Springer
The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …
[HTML][HTML] 3D turbulent reconnection: Theory, tests, and astrophysical implications
Magnetic reconnection, topological changes in magnetic fields, is a fundamental process in
magnetized plasmas. It is associated with energy release in regions of magnetic field …
magnetized plasmas. It is associated with energy release in regions of magnetic field …
Cosmological magnetic fields: their generation, evolution and observation
We review the possible mechanisms for the generation of cosmological magnetic fields,
discuss their evolution in an expanding Universe filled with the cosmic plasma and provide a …
discuss their evolution in an expanding Universe filled with the cosmic plasma and provide a …
The star formation rate of turbulent magnetized clouds: comparing theory, simulations, and observations
C Federrath, RS Klessen - The Astrophysical Journal, 2012 - iopscience.iop.org
The role of turbulence and magnetic fields is studied for star formation in molecular clouds.
We derive and compare six theoretical models for the star formation rate (SFR)—the …
We derive and compare six theoretical models for the star formation rate (SFR)—the …