Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...333..777m&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 333, Oct. 15, 1988, p. 777-787.
Astronomy and Astrophysics
Astronomy
31
Exosat Satellite, Pulsars, Radio Emission, Stellar Coronas, Supernova Remnants, X Ray Sources, Heao 2, Radio Sources (Astronomy), Spatial Distribution, Spectral Bands
Scientific paper
The authors report on the EXOSAT observation of the supernova remnant (SNR) G109.1-1.0+1E 2259+586 system. The spatial distribution of the X-ray emission as derived from the low-energy (<2 keV) data is very similar to that obtained from the Einstein Observatory. The various components of the source (SNR shell, pulsar, and jet) have different spectra. The jet is softer than the other components. The pulsar period was found to be 6.978725 s at the epoch of these observation, which implies a small positive Pwith respect to the value obtained from the Einstein data 4 years before. The data show no evidence for orbital motion. The central pulsating source is very peculiar in many respects and can hardly be interpreted in terms of a standard binary system.
Morini Marco
Robba Natale Renato
Smith Aaron
van der Klis Michael
No associations
LandOfFree
EXOSAT observations of the supernova remnant G109.1-1.0 and the X-ray pulsar 1E 2259+586 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with EXOSAT observations of the supernova remnant G109.1-1.0 and the X-ray pulsar 1E 2259+586, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and EXOSAT observations of the supernova remnant G109.1-1.0 and the X-ray pulsar 1E 2259+586 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1598162