JWST and ALMA Data Reveal Stellar Feedback Mechanisms in NGC 3256
Researchers have mapped pre-supernova pressure across 1,600 star clusters, providing a new template for understanding galaxy evolution.
No. 167
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Astronomers Detect Dual-Component Ultra-Fast Outflow in Distant Quasar
New observations of a hyper-luminous quasar reveal a complex, stratified wind structure that challenges existing models of black hole feedback.
No. 166
AAS 248 Sets Strategic Course for Next Decade of Astrophysics
The 248th meeting of the American Astronomical Society gathers researchers in Pasadena to define the scientific priorities and data infrastructure for the 2030s.
No. 164
Katalyst LINK Prepares for Rescue of NASA Swift Observatory
A commercial robotic spacecraft is set to launch in late June to extend the life of a critical gamma-ray burst telescope facing orbital decay.
No. 163
IIT Madras Unveils High-Resolution 3D Atlas of the Human Brainstem
The new ANCHOR project provides a multi-modal, cell-resolution map of the human brainstem to advance neurological research and clinical diagnostics.
No. 162
JWST observations reveal how supermassive black holes sustain their growth
New infrared data from the Centaurus cluster demonstrate how large-scale filamentary networks directly fuel the growth of central black holes.
No. 161
Supernova-driven winds identified as cause of early galaxy quiescence
New observations reveal how intense star formation and galactic collisions trigger powerful gas outflows that rapidly deplete fuel for future stellar growth.
No. 160
Astronomers detect earliest known flickering quasar from cosmic dawn
New research reveals a surprisingly mature supermassive black hole existing just 850 million years after the Big Bang.
No. 158
Magnetic Braking Resolves Longstanding Binary Star Formation Paradox
New supercomputer simulations reveal how interstellar magnetic fields strip rotational energy from protostars, explaining the compact orbits observed in binary systems.
No. 157
ALMA Imaging Reveals Persistent Outflow from Milky Way Central Black Hole
Researchers have identified a long-sought cone-shaped void in the galactic center, confirming that Sagittarius A* generates a continuous wind despite its quiescent state.
No. 156