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Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare
(SpringerDordrechtHolanda, 2011)
The cooling phase of Type I X-ray bursts observed with RXTE in 4U 1820-30 does not follow the canonical F-T^4 relation
(Wiley-blackwell Publishing, Inc, 2013-03)
We analysed the complete set of bursts from the neutron star low-mass X-ray binary 4U 1820-30 detected with the Rossi X-ray Timing Explorer (RXTE). We found that all are photospheric radius expansion bursts, and have similar ...
Spatial characterization of a flare using radio observations and magnetic field topology
(SpringerDordrechtHolanda, 2007)
Bright 30THz impulsive solar bursts
(Blackwell Publishing, 2015-06)
Impulsive 30THz continuum bursts have been recently observed in solar flares, utilizing small telescopes with a unique and relatively simple optical setup concept. The most intense burst was observed together with a GOES ...
Spectral Trends of Solar Bursts at Sub-THz Frequencies
(Springer, 2017-01)
Previous sub-THz studies were derived from single-event observations. We here analyze for the first time spectral trends for a larger collection of sub-THz bursts. The collection consists of a set of 16 moderate to small ...
Fast radio bursts and their gamma-ray or radio afterglows as Kerr-Newman black hole binaries
(IOP Publishing, 2016-07)
Fast radio bursts (FRBs) are radio transients lasting only about a few milliseconds. They seem to occur at cosmological distances. We propose that these events can originate in the collapse of the magnetospheres of Kerr-Newman ...
A two-zone approach to neutrino production in gamma-ray bursts
(Edp Sciences, 2014-02)
Context. Gamma-ray bursts (GRB) are the most powerful events in the universe. They are capable of accelerating particles to very high energies, so are strong candidates as sources of detectable astrophysical neutrinos. ...