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

Abstract

view Abstract Citations (38) References (25) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS A Kinematic Distance to the Supernova Remnant G33.6+0.1 Frail, D. A. ; Clifton, T. R. Abstract 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. Publication: The Astrophysical Journal Pub Date: January 1989 DOI: 10.1086/167056 Bibcode: 1989ApJ...336..854F Keywords: Astrometry; Nebulae; Pulsars; Supernova Remnants; Absorption Spectra; Emission Spectra; Hydrogen; Scattering Functions; Turbulence Effects; Very Large Array (Vla); Astrophysics; NEBULAE: INDIVIDUAL ALPHANUMERIC: G33.6; 0.1; NEBULAE: SUPERNOVA REMNANTS; PULSARS full text sources ADS | data products SIMBAD (2)