A distance determination for the supernova remnant G27.4+0.0 and its central X-ray source

Details A distance determination for the supernova remnant G27.4+0.0 and its central X-ray source A distance determination for the supernova remnant G27.4+0.0 and its central X-ray source

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aj....104.2189s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 104, no. 6, p. 2189-2192.

Astronomy and Astrophysics

Astronomy

38

Distance, Supernova Remnants, X Ray Sources, Absorption Spectra, Emission Spectra, H Ii Regions, Stellar Models, Very Large Array (Vla)

Scientific paper

We have determined the distance to the supernova remnant G27.4+0.0, one of the handful of remnants with a bright central X-ray source. H I absorption data obtained with the VLA toward the remnant and adjacent H II regions allow us to constrain the distance to G27.4+0.0 to lie between 6 and 7.5 kpc. We briefly discuss the implications of this result for the nature of the central source.

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