Results 91 to 100 of about 1,800,884 (153)

Comparing the interstellar and circumgalactic origin of gas in the tails of jellyfish galaxies

Simulations and observations have found long tails in ‘jellyfish galaxies’, which are commonly thought to originate from ram-pressure stripped gas of the interstellar medium (ISM) in the immediate galactic wake.
Sparre, Martin, Ewald Puchwein, Puchwein, Ewald, Christoph Pfrommer, Martin Sparre, Pfrommer, Christoph   +5 more
core   +1 more source

Magnetic Flux Plays an Important Role during a Black Hole X-Ray Binary Outburst in Radiative Two-temperature General Relativistic Magnetohydrodynamic Simulations

The Astrophysical Journal
Black hole (Bh) X-ray binaries cycle through different spectral states of accretion over the course of months to years. Although persistent changes in the Bh mass accretion rate are generally recognized as the most important component of state ...
M. T. P. Liska, N. Kaaz, K. Chatterjee, Razieh Emami, G. Musoke   +4 more
doaj   +1 more source

Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and <i>γ</i>-Ray Bursts. [PDF]

Front Astron Space Sci, 2021
Ruiz M, Shapiro SL, Tsokaros A.
europepmc   +1 more source

Binary Neutron Star Mergers: Magnetohydrodynamics and Neutrino Physics of General Relativistic Simulations of Binary Neutron Star Mergers [PDF]

Binary neutron star mergers are some of the most extreme events to happen in our universe. From observations of these mergers, we can obtain information about the properties of matter at densities much larger than those accessible within the solar system,
Knight, Alexander Lee
core   +1 more source

The Evolution of Substructure during Star Cluster Assembly

The Astrophysical Journal
Star cluster formation and assembly occur inside filamentary and turbulent molecular clouds, which imprint both spatial and kinematic substructure on the young cluster.
Edwin Laverde-Villarreal, Alison Sills, Claude Cournoyer-Cloutier, Veronica Arias Callejas   +3 more
doaj   +1 more source

A pebble accretion model for the formation of the terrestrial planets in the Solar System. [PDF]

Sci Adv, 2021
Johansen A, Ronnet T, Bizzarro M, Schiller M, Lambrechts M, Nordlund Å, Lammer H.   +6 more
europepmc   +1 more source

A hidden symmetry of the magnetohydrodynamical equations and invariant solutions

, 2014
Рассмотрена групповая структура уравнений магнитной гидродинамики. Для двухмерного случая с помощью скрытой конформной симметрии построены классы инвариантных решений.
Бабич, А.В.
core  

Magnetically driven outflows in the 3D common envelope evolution of massive stars

Recent three-dimensional magnetohydrodynamical simulations of the common envelope interaction have revealed the self-consistent formation of bipolar magnetically driven outflows.
Marco Vetter, Robert Andrassy, Andrassy, R., Mike Y. M. Lau, Roepke, F., Leidi, G., Moran-Fraile, J., Vetter, M., Ohlmann, S., Rüdiger Pakmor, Fabian R. N. Schneider, Pakmor, R., Friedrich K. Röpke, Giovanni Leidi, Sebastian Ohlmann, Damien Gagnier, Lau, M., Javier Morán-Fraile, Schneider, F., Gagnier, D.   +19 more
core   +1 more source

Interaction of a magnetized pulsar wind with its surroundings - MHD simulations of pulsar wind nebulae

, 2003
Magnetohydrodynamical simulations are presented of a magnetized pulsar wind interacting directly with the interstellar medium, or, in the case of a surrounding supernova remnant, with the associated freely expanding ejecta of the progenitor star. In both
E. van der Swaluw, van der Swaluw, E.
core   +1 more source

The Life and Times of Star-forming Cores: An Analysis of Dense Gas in the STARFORGE Simulations

The Astrophysical Journal
Dense gas in molecular clouds is an important signature of ongoing and future star formation. We identify and track dense cores in the starforge simulations, following the core evolution from birth through dispersal by stellar feedback for typical Milky ...
Stella S. R. Offner, Josh Taylor, Michael Y. Grudíc   +2 more
doaj   +1 more source