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| Query : 1996A&A...306L..49N |
1996A&A...306L..49N - Astronomy and Astrophysics, volume 306L49-51 (1996/2-3)
Evidence against the association of PSR B1706-44 with SNR G343.1-2.3.
NICASTRO L., JOHNSTON S. and KORIBALSKI B.
Abstract (from CDS):
An association between the supernova remnant SNR G343.1-2.3 and the pulsar PSR B1706-44 would imply a pulsar velocity greater than 1000km/s. Observations of the pulsar scintillation made with the Parkes radio telescope at 20 and 70cm indicate a velocity less than 50km/s. This fact, coupled with statistical arguments and the morphology of both the SNR and the pulsar plerion, shows that the association between the two objects is merely geometric projection.
Abstract Copyright: ∼
Journal keyword(s): pulsars: individual: PSR B1706-44 (PSR 1706-44) - stars: neutron - stars: kinematics - ISM: individual: SNR G343.1-2.3 (SNR 343.1-02.3) - ISM: supernova remnants - ISM: structure
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 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | SNR G343.1-02.3 | SNR | 17 08.0 | -44 16 | ~ | 82 | 1 | |||||
| 2 | PSR B1706-44 | Psr | 17 09 42.62000 | -44 29 12.0000 | 13.30 | ~ | 670 | 1 |
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