Erratum: ``Chandra View of the Unidentified TeV Gamma-Ray Source HESS J1804-216'' (ApJ, 652, L109 [2006])

Details Erratum: ``Chandra View of the Unidentified TeV Gamma-Ray Source HESS J1804-216'' (ApJ, 652, L109 [2006]) Erratum: ``Chandra View of the Unidentified TeV Gamma-Ray Source HESS J1804-216'' (ApJ, 652, L109 [2006])

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...665l..83c&link_type=abstract

The Astrophysical Journal, Volume 665, Issue 1, pp. L83-L83.

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Scientific paper

After the publication of our Letter, new observations of PSR J1803-2137 (W. F. Brisken et al. [ApJ, 652, L109 [2006]]) yielded a radio position of the pulsar (R.A. = 18h03m51.4105s, decl. = -21°37'07.351") that is significantly different from the position (R.A. = 18h03m51.333s, decl. = -21°36'27" G. Hobbs et al. [ApJ, 652, L109 [2006]]) adopted for the Letter. The new position puts the pulsar right in the extended X-ray feature that we detected (with the center of gravity located at R.A. = 18h03m51.411s, decl. = -21°37'07.37"), which strengthens the argument for its being a pulsar wind nebula. No other conclusions are affected.

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