Search Results - "Araudo, A. T"
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1
Ultrahigh energy cosmic rays from shocks in the lobes of powerful radio galaxies
Published in Monthly notices of the Royal Astronomical Society (01-02-2019)Get full text
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2
Fornax A, Centaurus A, and other radio galaxies as sources of ultrahigh energy cosmic rays
Published in Monthly notices of the Royal Astronomical Society. Letters (01-09-2018)“…ABSTRACT The origin of ultrahigh energy cosmic rays (UHECRs) is still unknown. It has recently been proposed that UHECR anisotropies can be attributed to…”
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Gamma-Ray Variability from Wind Clumping in High-Mass X-Ray Binaries with Jets
Published in The Astrophysical journal (01-05-2009)“…In the subclass of high-mass X-ray binaries known as 'microquasars,' relativistic hadrons in the jets launched by the compact object can interact with cold…”
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4
Cosmic-ray acceleration by relativistic shocks: limits and estimates
Published in Monthly notices of the Royal Astronomical Society (01-01-2018)Get full text
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5
Gamma-ray emission from massive stars interacting with active galactic nuclei jets
Published in Monthly notices of the Royal Astronomical Society (21-12-2013)“…Dense populations of stars surround the nuclear regions of galaxies. In active galactic nuclei, these stars can interact with the relativistic jets launched by…”
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6
Cosmic ray acceleration in hydromagnetic flux tubes
Published in Monthly notices of the Royal Astronomical Society (21-08-2019)Get full text
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7
Amplification of perpendicular and parallel magnetic fields by cosmic ray currents
Published in Monthly notices of the Royal Astronomical Society (01-08-2017)“…Abstract Cosmic ray (CR) currents through magnetized plasma drive strong instabilities producing amplification of the magnetic field. This amplification helps…”
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Modeling the Prompt Optical Emission of GRB 180325A: The Evolution of a Spike from the Optical to Gamma Rays
Published in The Astrophysical journal (10-02-2021)“…The transition from prompt to afterglow emission is one of the most exciting and least understood phases in gamma-ray bursts (GRBs). Correlations among…”
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PARTICLE ACCELERATION AND MAGNETIC FIELD AMPLIFICATION IN THE JETS OF 4C74.26
Published in The Astrophysical journal (20-06-2015)“…ABSTRACT We model the multi-wavelength emission in the southern hotspot of the radio quasar 4C74.26. The synchrotron radio emission is resolved near the shock…”
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Cosmic Ray Acceleration by Relativistic Shocks: Limits and Estimates
Published 22-09-2017“…We examine limits to the energy to which cosmic rays can be accelerated by relativistic shocks, showing that acceleration of light ions as high as 100 EeV is…”
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Extremely violent optical microvariability in blazars: fact or fiction?
Published in Monthly notices of the Royal Astronomical Society (01-01-2007)“…Variability amplitudes larger than 1 mag over time-scales of a few tens of minutes have recently been reported in the optical light curves of several blazars…”
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Massive protostars as gamma-ray sources
Published 30-11-2009“…Massive protostars have associated bipolar outflows with velocities of hundreds of km s$^{-1}$. Such outflows can produce strong shocks when interact with the…”
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Gamma-ray variability from wind clumping in HMXBs with jets
Published 13-02-2009“…Astrophys.J.696:690-693,2009 In the subclass of high-mass X-ray binaries known as "microquasars", relativistic hadrons in the jets launched by the compact…”
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14
GAMMA-RAY VARIABILITY FROM WIND CLUMPING IN HIGH-MASS X-RAY BINARIES WITH JETS
Published in The Astrophysical journal (01-05-2009)“…In the subclass of high-mass X-ray binaries known as 'microquasars', relativistic hadrons in the jets launched by the compact object can interact with cold…”
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15
Gamma-ray emission from massive star forming regions
Published 13-05-2008“…Int.J.Mod.Phys.D17:1889-1894,2008 Recent radio observations support a picture for star formation where there is accretion of matter onto a central protostar…”
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Gamma-ray emission from massive young stellar objects
Published 22-08-2007“…Astron.Astrophys.476:1289,2007 Massive stars form in dense and massive molecular cores. The exact formation mechanism is unclear, but it is possible that some…”
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17
Using gamma-rays to probe the clumped structure of stellar winds
Published 10-08-2007“…Gamma-rays can be produced by the interaction of a relativistic jet and the matter of the stellar wind in the subclass of massive X-ray binaries known as…”
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