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Optical Image (3 arcmin on a side, red = DSS 2 IR, green = DSS 2 red, blue = DSS 2 blue · Crab Weighted Monthly Mosaic Lightcurve for SWIFT J1419.0-2639
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Help | Advanced Search · arXiv is a free distribution service and an open-access archive for nearly 2.4 million scholarly articles in the fields of physics, mathematics, computer science, quantitative biology, quantitative finance, statistics, electrical engineering and systems science, and ...
The radio quasar NVSS J141922−083830 (J1419−0838) was initially classified as an uncategorised blazar-type object, following its detection in the γ $\gamma $ -ray band with the Fermi space telescope. Later, using multi-waveband observations and modeling, its was found to be a flat-spectrum ...
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July 1, 2020 - Nonetheless, no radio flare observation has been reported to date. Here we show that the radio transient FIRST J1419+3940, first observed in 1993 and still detectable, could have originated from a neutron star merger. We carry out numerical simulations of neutron star merger ejecta to demonstrate ...
July 4, 2020 - Access 160+ million publications and connect with 25+ million researchers. Join for free and gain visibility by uploading your research.
Access 160+ million publications and connect with 25+ million researchers. Join for free and gain visibility by uploading your research.
Nonetheless, no radio flare observation has been reported to date. Here we show that the radio transient FIRST J1419+3940, first observed in 1993 and still detectable, could have originated from a neutron star merger. We carry out numerical simulations of neutron star merger ejecta to demonstrate ...
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