(1) Radio spectral index variations of the SNR HB3 (2) Radio spectral index study of the SNRs OA184 and VRO42.05.01
National Astronomical Observatories, CAS, Beijing 100012, PR China e-mail: email@example.com
2 Department of Physics & Astronomy, University of Calgary, Calgary, Alberta T2N 1N4, Canada
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