A&A 451, 991-991 (2006)
(1) Radio spectral index variations of the SNR HB3 (2) Radio spectral index study of the SNRs OA184 and VRO42.05.01W. W. Tian1 and D. A. Leahy2
1 National Astronomical Observatories, CAS, Beijing 100012, PR China
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 (not ) for HB3, (not ) for OA184 and (not ) 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 arcmin not 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