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Query : 2004A&A...420..937V |
2004A&A...420..937V - Astronomy and Astrophysics, volume 420, 937-944 (2004/6-4)
An evolutionary model for pulsar-driven supernova remnants. A hydrodynamical model.
VAN DER SWALUW E., DOWNES T.P. and KEEGAN R.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): pulsars: general - stars: supernova remnants - shocks waves - hydrodynamics
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 | NGC 2060 | SNR | 05 37 51.4466169456 | -69 10 23.947092084 | 9.69 | 9.59 | ~ | 360 | 2 | |||
2 | SNR G327.1-01.1 | SNR | 15 54 32.3 | -55 03 44 | ~ | 99 | 1 | |||||
3 | SNR G034.6-00.5 | SNR | 18 56 10.650 | +01 13 21.30 | ~ | 964 | 2 | |||||
4 | SNR G068.8+02.6 | SNR | 19 52 55 | +32 54.2 | ~ | 352 | 1 |
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