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Query : 1999A&A...352..712G |
1999A&A...352..712G - Astronomy and Astrophysics, volume 352, 712-722 (1999/12-2)
The nature of the Vela X-ray ``jet". The Rayleigh-Taylor instability and the origin of filamentary structures in the Vela supernova remnant.
GVARAMADZE V.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): shock waves - stars: pulsars: individual: Vela X - ISM: bubbles - ISM: supernova remnants - X-rays: ISM
Simbad objects: 3
Number of rows : 3 |
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 | NAME Vela X | Psr | 08 33 08.880 | -45 11 24.36 | ~ | 282 | 1 | |||||
2 | NAME Vela XYZ | Rad | 08 34.0 | -45 50 | ~ | 1231 | 2 | |||||
3 | NAME Cyg Loop | SNR | 20 51.0 | +30 40 | ~ | 913 | 0 |
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