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Query : 2017ApJ...849L..22W |
2017ApJ...849L..22W - Astrophys. J., 849, L22-L22 (2017/November-2)
When disorder looks like order: a new model to explain Radial magnetic fields in young supernova remnants.
WEST J.L., JAFFE T., FERRAND G., SAFI-HARB S. and GAENSLER B.M.
Abstract (from CDS):
Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.
Journal keyword(s): cosmic rays - ISM: magnetic fields - ISM: supernova remnants - polarization - radio continuum: ISM - radio continuum: ISM
Simbad objects: 4
Number of rows : 4 |
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 | SN 1572A | SN* | 00 25 21.5 | +64 08 27 | B8 | 1188 | 1 | |||||
2 | NAME Lupus SN | SNR | 15 02 22.1 | -42 05 49 | ~ | 1329 | 1 | |||||
3 | NAME Kepler SNR | Rad | 17 30 40.5 | -21 29 14 | ~ | 795 | 4 | |||||
4 | 3C 461 | BL? | 23 23 24.000 | +58 48 54.00 | 14.30 | ~ | 2792 | 1 |
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