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Accreting Binaries
Accretion disks
Ambipolar diffusion
Artificial Intelligence
Black holes
Bright AGNs
Brown dwarfs
CGM
Cosmic Dawn
Current Sheets
Dark energy
Dark matter
Einstein
Electromagnetic and Gravitational Wave Signals
Eve of Roman
FRB Dispersion and Scattering
First stars
Galactic Center
Galaxy Clusters
Galaxy Formation
Galaxy formation process
Gravitational waves
ISM
Kolmogorov
LIGO-Virgo-KAGRA
LMC
Local Universe
Major mergers
Microlensing
Milky way
Multiverse time travel
Neutrinos
Neutron Stars
Nuclear Reactions
Particle Heating
Photo-Ionized Gas
Photometric redshifts
Plasma processes
Plasmoid Instability
Precision Measurement
Proto-Planetary Disks
Sky surveys
Solar System Oceans
Spacetime
Spacetime disturbances
Star Formation
Star Forming Regions
Stars
Supermassive black holes
The Cosmic Neutrino Background
Time-Resolved Photometric Surveys
Turbulent collapsing clouds
Wind Blown Bubbles
metal-poor stars

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Four colorful scientific heat maps with axes labeled x and y, each showing patterns of fragmentation and star formation, with color bars on the right displaying a logarithmic scale and overlaid contour lines.

July 3, 2025

Stellar Evolution and Pollution in AGN Disks

Douglas Lin, UC Santa Cruz

Four panels show colorful scientific simulations of space clouds with swirling blue, white, and yellow patterns. Captions compare effects of gravity, turbulence, magnetic fields, and jets on star formation rates and efficiency.

June 19, 2025

Ambipolar diffusion and the mass-to-flux ratio in turbulent collapsing clouds

Aris Tritsis, EPFL

A colorful abstract background with stylized faces, overlaid by an image of the Milky Way galaxy and text: The unquiet neighbour: how the LMC bugs the Milky Way by Eugene Vasiliev, University of Barcelona, 10 April 2023.

June 17, 2025

The Unquiet Neighbour: How the LMC bugs the Milky Way

Eugene Vasiliev, University of Surrey

March 26, 2015

The morphology of the Milky Way and spiral galaxies

The arm structure of the Milky Way remains somewhat of an unknown, with observational studies hindered by our location within the Galactic disk. We present the results of a project aimed at constraining the global structure of the Milky Way through numerous numerical simulations and synthetic observations.