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2013MNRAS.435..879T - Mon. Not. R. Astron. Soc., 435, 879-884 (2013/October-2)
The neutron star born in the Antlia supernova remnant.
TETZLAFF N., TORRES G., NEUHAUSER R. and HOHLE M.M.
Abstract (from CDS):
We find the pulsar PSR J0630-2834 to be the best candidate for a common origin with the Antlia SNR. In that scenario, the SNR is ~1.2Myr old and is presently located at a distance of ~138pc. We consider the runaway star HIP 47155 a former companion candidate to PSR J0630-2834. The encounter time and place is consistent with both stars being ejected from the Antlia SNR. We measured the radial velocity of HIP 47155 as 32.42±0.70km/s.
Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)
Journal keyword(s): pulsars: individual: PSR J0630-2834
Simbad objects: 17
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