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Query : 2018MNRAS.478.2074B |
2018MNRAS.478.2074B - Mon. Not. R. Astron. Soc., 478, 2074-2085 (2018/August-1)
A laminar model for the magnetic field structure in bow-shock pulsar wind nebulae.
BUCCIANTINI N.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): MHD - polarization - radiation mechanisms: non-thermal - relativistic processes - ISM: supernova remnants
Simbad objects: 6
Number of rows : 6 |
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 | M 1 | SNR | 05 34 30.9 | +22 00 53 | ~ | 6193 | 1 | |||||
2 | NAME Geminga | Psr | 06 33 54.153 | +17 46 12.91 | ~ | 1222 | 0 | |||||
3 | IGR J11014-6103 | gam | 11 01 45.05 | -61 01 40.3 | ~ | 53 | 0 | |||||
4 | NAME the Frying Pan Handle | Rad | 14 37 01.91 | -59 59 01.4 | ~ | 6 | 1 | |||||
5 | NAME Mouse | Rad | 17 47 15.78 | -29 58 01.0 | ~ | 111 | 1 | |||||
6 | PSR B2223+65 | Psr | 22 25 52.8627 | +65 35 36.371 | ~ | 323 | 0 |
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