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Query : 2019MNRAS.484.1475T |
2019MNRAS.484.1475T - Mon. Not. R. Astron. Soc., 484, 1475-1486 (2019/April-1)
Modelling the bow shock Pulsar Wind Nebulae propagating through a non-uniform ISM.
TOROPINA O.D., ROMANOVA M.M. and LOVELACE R.V.E.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): magnetic fields - MHD - stars: neutron - stars: pulsars
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 | PSR B0740-28 | Psr | 07 42 49.0730 | -28 22 43.510 | ~ | 407 | 0 | |||||
3 | PSR J1509-5850 | Psr | 15 09 27.153 | -58 50 56.05 | ~ | 118 | 0 | |||||
4 | NAME Mouse | Rad | 17 47 15.78 | -29 58 01.0 | ~ | 111 | 1 | |||||
5 | PSR J1747-2958 | Psr | 17 47 15.869 | -29 58 00.93 | ~ | 131 | 1 | |||||
6 | PSR B2223+65 | Psr | 22 25 52.8627 | +65 35 36.371 | ~ | 323 | 0 |
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