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Title:
A kinematic distance to the supernova remnant G33.6+0.1
Authors:
Frail, D. A.; Clifton, T. R.
Affiliation:
AA(Toronto, University, Canada), AB(California, University, Berkeley; Manchester, Victoria University, Jodrell Bank, England)
Publication:
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 15, 1989, p. 854-860. Research supported by NSERC. (ApJ Homepage)
Publication Date:
01/1989
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
ASTROMETRY, NEBULAE, PULSARS, SUPERNOVA REMNANTS, ABSORPTION SPECTRA, EMISSION SPECTRA, HYDROGEN, SCATTERING FUNCTIONS, TURBULENCE EFFECTS, VERY LARGE ARRAY (VLA)
DOI:
10.1086/167056
Bibliographic Code:
1989ApJ...336..854F

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.

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