2017ApJ...836..159D


C.D.S. - SIMBAD4 rel 1.7 - 2021.04.14CEST13:22:00

2017ApJ...836..159D - Astrophys. J., 836, 159-159 (2017/February-3)

Revised predictions of neutrino fluxes from pulsar wind nebulae.

DI PALMA I., GUETTA D. and AMATO E.

Abstract (from CDS):

Several pulsar wind nebulae (PWN) have been detected in the TeV band in the last decade. TeV emission is typically interpreted in a purely leptonic scenario, but this often requires that the magnetic field in the nebula be much lower than the equipartition value, as well as the assumption of an enhanced density of target radiation at IR frequencies. In this work, we consider the possibility that, in addition to the relativistic electrons and positrons, relativistic hadrons are also present in these nebulae. Assuming that some of the emitted TeV photons are of hadronic origin, we compute the associated flux of ∼1–100 TeV neutrinos. We use IceCube non-detection to put constraints on the fraction of TeV photons that might be contributed by hadrons and estimate the number of neutrino events that can be expected from these sources in ANTARES and KM3Net.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): gamma rays: ISM - ISM: supernova remnants - neutrinos - neutrinos

Errata: erratum vol. 848, art. 74 (2017)

Simbad objects: 29

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Number of rows : 29

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 SNR G119.5+10.2 SNR 00 06.6 +72 47           ~ 238 1
2 V* CM Tau Psr 05 34 31.93830 +22 00 52.1758           ~ 4879 1
3 M 1 SNR 05 34 31.94 +22 00 52.2           ~ 5722 4
4 NGC 2060 SNR 05 37 51.4470067818 -69 10 23.957283532   9.69 9.59     ~ 327 2
5 NAME Vela XYZ Rad 08 34.0 -45 50           ~ 1137 2
6 FGES J1023.3-5747 gam 10 23 15.18313 -57 46 34.7840           ~ 53 0
7 PSR J1301-6305 Psr 13 01 45.76 -63 05 33.9           ~ 105 2
8 PSR J1357-6429 Psr 13 57 02.525 -64 29 29.89           ~ 123 1
9 PSR J1418-6058 Psr 14 18 42.725 -60 58 01.89           ~ 106 0
10 PSR J1420-6048 Psr 14 20 08.190 -60 48 14.85           ~ 165 0
11 PSR J1459-60 Psr 14 59 30.222 -60 53 19.87           ~ 44 0
12 3A 1510-590 Psr 15 13 17.000 -59 04 54.00           ~ 382 3
13 PSR B1509-58 Psr 15 13 55.52 -59 08 08.8     13.06     ~ 805 1
14 AJG 44 Psr 16 17 33.000 -51 02 00.00           ~ 465 3
15 3FHL J1633.0-4746e HXB 16 32 01.87 -47 52 28.3           O8I 151 3
16 3EG J1639-4702 gam 16 40 30.0 -46 33 00           ~ 137 2
17 HESS J1708-443 gam 17 07 59.53847 -44 17 19.0460           ~ 12 0
18 SNR G000.9+00.1 SNR 17 47.3 -28 09           ~ 174 1
19 HESS J1809-193 gam 18 10 31 -19 18.0           ~ 44 1
20 NAME AGPS 273.4-17.8 SNR 18 13 35.05 -17 49 58.1           ~ 95 2
21 PSR B1823-13 Psr 18 26 13.06 -13 34 48.1           ~ 363 1
22 HESS J1831-098 gam 18 31.4 -09 54           ~ 9 0
23 SNR G021.5-00.9 SNR 18 33 33.612 -10 34 07.69           ~ 405 1
24 SNR G023.3-00.3 SNR 18 34 51.80 -08 44 38.2           ~ 195 0
25 PSR J1838-0655 Psr 18 38 03.13 -06 55 33.4           ~ 83 1
26 ARGO J1839-0627 Psr 18 40 55.0 -05 33 00           ~ 47 1
27 SNR G029.7-00.2 SNR 18 46 25.5 -02 59 14           ~ 304 2
28 ARGO J1912+1026 gam 19 12 +10.1           ~ 32 0
29 SNR G054.1+00.3 SNR 19 30 31 +18 52.0           ~ 198 1

    Equat.    Gal    SGal    Ecl

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2021.04.14-13:22:00

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