Results 71 to 80 of about 207,256 (183)
The Astrophysical Journal4C+29.30 is a postmerger galaxy hosting a rejuvenated active galactic nucleus (AGN) with a complex multiscale radio morphology, making it an ideal laboratory to study the interplay between different AGN feedback modes.
Xiao Cao +7 more
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Modeling the Milky Way wind: Supernova-driven outflows accelerate HI clouds near the Galactic center
Astronomy & AstrophysicsMultiwavelength observations, from radio to X-rays, have revealed the presence of multiphase high-velocity gas near the center of the Milky Way likely associated with powerful galactic outflows. This region offers a unique laboratory to study the physics
Afruni Andrea +4 more
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When are galactic winds molecular?
Monthly Notices of the Royal Astronomical SocietyABSTRACT The molecular phase of supernova-driven outflows originates from the cold, molecular gas in the disc of a star-forming galaxy, and may carry a substantial fraction of the wind mass flux in some galaxies, but it remains poorly understood.
Aditi Vijayan, Mark R Krumholz
openaire +2 more sources
Dust Evolution in Simulated Multiphase Galactic Outflows
The Astrophysical JournalWe present the first large-scale, high-resolution simulations of dusty, star formation feedback-driven galactic outflows. Using the Cholla hydrodynamics code, we investigate dust sputtering in these environments for grains ranging in size from 1 to 0.001
Helena M. Richie, Evan E. Schneider
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On the Stability of Interstellar Neutral Hydrogen Clouds at Large Z-heights
The Astrophysical JournalGalactic neutral hydrogen (H i ) data drawn from several large-scale surveys have been used to study 32 small clouds found between Galactic longitudes 70° and 140° and latitudes −20° and −45°.
G. L. Verschuur
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The Astrophysical JournalGalactic outflows driven by rapidly accreting quasars at high redshift are widely expected to play a key role in the short- and long-term future evolution of their host galaxies.
Justin S. Spilker +6 more
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Hydrodynamical Simulation of Wind Production from Hot Accretion Flows in Tidal Disruption Events
The Astrophysical JournalWind is a key mechanism for supermassive black hole (SMBH) feedback to their host galaxies. In tidal disruption events (TDEs), black holes spend most of their time accreting at highly sub-Eddington rates, implying that feedback from persistent sub ...
Mingjun Liu +7 more
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Cosmic-Ray-driven Galactic Winds with Resolved Interstellar Medium and Ion-neutral Damping
The Astrophysical JournalFeedback processes in galaxies dictate their structure and evolution. Baryons can be cycled through stars, which inject energy into the interstellar medium in supernova explosions, fueling multiphase galactic winds.
Brandon Sike +4 more
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Shockingly Effective: Cluster Winds as Engines of Feedback in Starburst Galaxy VV 114
The Astrophysical JournalWe present high-resolution Keck Cosmic Web Imager and MUSE integral field unit spectroscopy of VV 114, a local IR-luminous merger undergoing a vigorous starburst and showing evidence of galactic-scale feedback. The high-resolution data allow for spectral
Justin A. Kader +31 more
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