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- W1996306525 abstract "view Abstract Citations (43) References (19) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The PSR 1800-21/G8.7-0.1 Association: A View from ROSAT Finley, John P. ; Oegelman, Hakki Abstract We present the first imaging X-ray observation of the W30 complex which contains the Galactic SNR G8.7-0.1 and the young radio pulsar PSR 1800-21 as well as a number of discrete ultracompact H II regions. The pulsar PSR 1800-21 is detected as a count rate of 1.5 +/- 0.5/ks and diffuse emission from the northern extent of G8.7-0.1 observed. The data support an association of G8.7-0.1 and PSR 1800-21, and the peculiar morphology can be explained if the supernova which gave birth to PSR 1800-21 occurred within, or very near, a molecular cloud. The suggested scenario removes the requirement of a large transverse velocity for the pulsar, one of the greatest dificulties with the association. Publication: The Astrophysical Journal Pub Date: October 1994 DOI: 10.1086/187563 Bibcode: 1994ApJ...434L..25F Keywords: Emission Spectra; Morphology; Supernova Remnants; X Ray Astronomy; X Ray Imagery; H Ii Regions; Molecular Clouds; Pulsars; Rosat Mission; X Ray Telescopes; Astrophysics; ISM: SUPERNOVA REMNANTS; STARS: NEUTRON; STARS: PULSARS: INDIVIDUAL ALPHANUMERIC: PSR 1800-21; X-RAYS: STARS full text sources ADS | data products SIMBAD (3) HEASARC (1)" @default.
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- W1996306525 date "1994-10-01" @default.
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- W1996306525 title "The PSR 1800-21/G8.7-0.1 association: A view from ROSAT" @default.
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