A kinematic distance to the supernova remnant G33.6+0.1

Details A kinematic distance to the supernova remnant G33.6+0.1 A kinematic distance to the supernova remnant G33.6+0.1

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336..854f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 15, 1989, p. 854-860. Research supported by NSERC.

Other

27

Astrometry, Nebulae, Pulsars, Supernova Remnants, Absorption Spectra, Emission Spectra, Hydrogen, Scattering Functions, Turbulence Effects, Very Large Array (Vla)

Scientific paper

Neutral hydrogen absorption spectra have been made toward the supernova remnant G33.6+0.1 and two nearby points sources in the field. These observations are used with published data for the pulsar PSR 1849+00 to determine kinematic distances and to resolve the relative geometry between these objects. G33.6+0.1 was found to be at a distance of 10 + or - 2 kpc, and lies in the foreground of the other objects studied. The possibility that G33.6+0.1 is the source of the heavy scattering observed in this direction is investigated.

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