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Issue A&A
Volume 451, Number 3, June I 2006
Page(s) 991 - 991
Section Interstellar and circumstellar matter
DOI http://dx.doi.org/10.1051/0004-6361:20042431e



A&A 451, 991-991 (2006)
DOI: 10.1051/0004-6361:20042431e

Erratum

(1) Radio spectral index variations of the SNR HB3 (2) Radio spectral index study of the SNRs OA184 and VRO42.05.01

W. W. Tian1 and D. A. Leahy2

1  National Astronomical Observatories, CAS, Beijing 100012, PR China
    e-mail: tww@ns.bao.ac.cn
2  Department of Physics & Astronomy, University of Calgary, Calgary, Alberta T2N 1N4, Canada

((1) A&A, 436, 187-193 (2005), DOI: 10.1051/0004-6361:20042431 (2) A&A, 440, 929-936 (2005), DOI: 10.1051/0004-6361:20053392)

For both above papers, there were mistakes in calculation of the spectral index errors in Tables 3 which have been corrected in the following replacement tables respectively. Therefore the integrated flux density based spectral index error cited in the text changes to $0.34\pm0.25$ (not $0.34\pm0.15$) for HB3, $0.25\pm0.08$ (not $0.25\pm0.03$) for OA184 and $0.36\pm0.10$ (not $0.36\pm0.06$) for VRO42.05.01. The correct beamwidth for the 2695 MHz effelsberg 100-m in Table 4 (for the both papers) and 5 (only for the second paper) is $4.3 \times 4.3$ arcmin not $3.4 \times 3.4$ arcmin. None of the above corrections affect our discussions and conclusions in the two papers.


Key words: ISM: individual objects: HB3 -- ISM: individual objects: OA184 -- ISM: individual objects: VRO42.05.01 -- ISM: supernova remnants -- radio continuum: ISM -- errata, addenda




© ESO 2006

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