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Query : 2019MNRAS.484.5755O |
2019MNRAS.484.5755O - Mon. Not. R. Astron. Soc., 484, 5755-5770 (2019/April-3)
Full-3D relativistic MHD simulations of bow shock pulsar wind nebulae: dynamics.
OLMI B. and BUCCIANTINI N.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): MHD - relativistic processes - turbulence - methods: numerical - pulsars: general - ISM: supernova remnants
Simbad objects: 2
Number of rows : 2 |
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 | ~ | 6198 | 1 | |||||
2 | NAME Vela XYZ | Rad | 08 34.0 | -45 50 | ~ | 1231 | 2 |
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