Results 121 to 130 of about 89,220 (323)

Effect of Background Magnetic Field on Ion Weibel Instability With High‐Intensity Short‐Pulse Lasers

open access: yesContributions to Plasma Physics, EarlyView.
ABSTRACT The effect of finite background magnetic field on magnetic field amplification by Weibel instability using high‐intensity short‐pulse lasers is investigated. We consider Weibel instability for counter‐streaming sub‐relativistic plasma flows generated by shooting pure carbon targets with short‐pulse lasers.
Taiki Jikei   +3 more
wiley   +1 more source

Active Galactic Nucleus Star Dynamics Under the Influence of Outflow–Ambient Interactions

open access: yesThe Astrophysical Journal
Stars with outflows interacting with ambient gas experience accelerations arising from the gravitational feedback induced by the interaction structure.
Muxin Liu, Lile Wang, Peng Peng
doaj   +1 more source

RESOLVING THE ACTIVE GALACTIC NUCLEUS AND HOST EMISSION IN THE MID-INFRARED USING A MODEL-INDEPENDENT SPECTRAL DECOMPOSITION [PDF]

open access: yes, 2015
We present results on the spectral decomposition of 118 Spitzer Infrared Spectrograph (IRS) spectra from local active galactic nuclei (AGNs) using a large set of Spitzer/IRS spectra as templates.
A. Hernán-Caballero   +8 more
semanticscholar   +1 more source

The Fermi Bubbles. I. Possible Evidence for Recent AGN Jet Activity in the Galaxy

open access: yes, 2012
The Fermi Gamma-ray Space Telescope reveals two large gamma-ray bubbles in the Galaxy, which extend about 50 degrees (~ 10 kpc) above and below the Galactic center (GC) and are symmetric about the Galactic plane.
Bland-Hawthorn   +29 more
core   +1 more source

Adverse Outcome Pathways Applied to Space Radiation Research

open access: yesEnvironmental and Molecular Mutagenesis, EarlyView.
ABSTRACT Long‐duration spaceflight exposes astronauts to various stressors that can alter human physiology, potentially causing immediate and long‐term health effects. These stressors can damage biomolecules, cells, tissues, and organs, leading to adverse outcomes.
Vinita Chauhan   +18 more
wiley   +1 more source

AGN/Starburst Connection

open access: yesActa Polytechnica CTU Proceedings, 2014
Two main physical processes characterize the activity in the nuclear region of active galaxies: an intense star formation (starburst, SB) and an Active Galactic Nucleus (AGN).
Eleonora Sani
doaj   +1 more source

Star formation history in barred spiral galaxies – active galactic nucleus feedback [PDF]

open access: yes, 2017
We present a numerical study of the impact of AGN accretion and feedback on the star formation history of barred disc galaxies. Our goal is to determine whether the effect of feedback is positive (enhanced star formation) or negative (quenched star ...
Fidèle Robichaud   +4 more
semanticscholar   +1 more source

Illuminating Satellite Cells: Light Sheet Fluorescence Microscopy for 3D Imaging of Murine Skeletal Muscles Damaged by Ex Vivo Forced Eccentric Contraction

open access: yesMicroscopy Research and Technique, EarlyView.
This study presents the light sheet fluorescence microscopy (LSFM) as a tool for 3D‐imaging of whole skeletal muscle to reveal satellite cells (SCs), the muscle stem cells that activate following damage to repair injured tissue. After tissue clearing and whole‐mount staining process aimed to enable optical access and specific cell labeling (1), murine ...
Rachele Garella   +11 more
wiley   +1 more source

Accretion of Active Galactic Nucleus Stars Under the Influence of Disk Geometry

open access: yesThe Astrophysical Journal
Massive stars can form within or be captured by active galactic nucleus disks, influencing both the thermal structure and metallicity of the disk environment.
Yi-Xian Chen   +2 more
doaj   +1 more source

Factors Determining Variability Time in Active Galactic Nucleus Jets [PDF]

open access: yesPublications of the Astronomical Society of Australia, 2002
AbstractThe relationship between observed variability time and emission region geometry is explored for the case of emission by relativistic jets.The approximate formula for the jet-frame size of the emission region, R′ = DcΔtobs, is shown to lead to large systematic errors when used together with observed luminosity and assumed or estimated Doppler ...
openaire   +5 more sources

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