2019ApJ...887..202W


Query : 2019ApJ...887..202W

2019ApJ...887..202W - Astrophys. J., 887, 202-202 (2019/December-3)

Consequences of energetic magnetar-like outbursts of nearby neutron stars: 14C events and the cosmic electron spectrum.

WANG F.Y., LI X., CHERNYSHOV D.O., HUI C.Y., ZHANG G.Q. and CHENG K.S.

Abstract (from CDS):

Four significant events of rapid 14C increase have taken place within the past several thousand years. The physical origin of these rapid increases is still a mystery but must be associated with extremely energetic cosmic processes. Pulsars are highly magnetized neutron stars that emit a beam of electromagnetic radiations. Any sudden release of the energy stored in the magnetic multipole field will trigger outbursts similar to the giant flares of magnetars. Here we show that the relativistic outflow from the outbursts of a nearby pulsar interacting with the interstellar medium generates a shock, which accelerates electrons to trillions of electron volts. The high-energy photons from synchrotron emission of the shock interact with Earth's atmosphere, producing the cosmogenic nuclide 14C, which can cause the rapid 14C increases discovered in tree rings. These same relativistic electrons can account for a significant fraction of the cosmic electron spectrum in the trillion electron volts energy range, as observed by space-borne satellites. Since these outburst events can significantly affect our environment, monitoring nearby pulsars for such outbursts may be important in the future.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): High-energy cosmic radiation - Magnetars

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 NAME Geminga Psr 06 33 54.153 +17 46 12.91           ~ 1222 0
2 PSR B0656+14 Psr 06 59 48.1960 +14 14 19.400   24.85 24.90     ~ 869 1
3 PSR B0834+06 Psr 08 37 05.642 +06 10 14.56           ~ 437 0
4 PSR B1055-52 Psr 10 57 59.0450 -52 26 56.330           ~ 725 0
5 PSR J1119-6127 Psr 11 19 14.30 -61 27 49.5           ~ 404 1
6 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2003 0
7 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1240 2
8 PSR J1846-0258 Psr 18 46 24.94 -02 58 30.1           ~ 347 2
9 RX J1856.6-3754 Psr 18 56 35.11 -37 54 30.5     25.7     ~ 437 0

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