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Query : 2017MNRAS.464..940F |
2017MNRAS.464..940F - Mon. Not. R. Astron. Soc., 464, 940-945 (2017/January-1)
Numerically modelling the Cygnus Loop as a remnant evolved in an anisotropic cavity.
FANG J., YU H. and ZHANG L.
Abstract (from CDS):
Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): hydrodynamics - methods: numerical - ISM: individual objects: Cygnus Loop - ISM: supernova remnants - ISM: supernova remnants
Simbad objects: 7
Number of rows : 7 |
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 | * omi Cet | Mi* | 02 19 20.79210 | -02 58 39.4956 | 7.63 | 6.53 | 5.03 | M5-9IIIe+DA | 1525 | 0 | ||
2 | NAME Vela Jr SN | BL? | 08 52.0 | -46 20 | ~ | 474 | 2 | |||||
3 | NAME Lupus SN | SNR | 15 02 22.1 | -42 05 49 | ~ | 1326 | 1 | |||||
4 | SNR G352.7-00.1 | Rad | 17 27 43 | -35 06.5 | ~ | 71 | 1 | |||||
5 | SNR G001.9+00.3 | SNR | 17 48 46.0 | -27 09 52 | ~ | 209 | 1 | |||||
6 | NAME Cyg Loop | SNR | 20 51.0 | +30 40 | ~ | 912 | 0 | |||||
7 | 3C 461 | BL? | 23 23 24.000 | +58 48 54.00 | 14.30 | ~ | 2780 | 1 |
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