[https://doi.org/10.1051/0004-6361:20053392]
[https://doi.org/10.1051/0004-6361:20042431]
| Issue |
A&A
Volume 451, Number 3, June I 2006
|
|
|---|---|---|
| Page(s) | 991 - 991 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361:20042431e | |
| Published online | 04 May 2006 | |
(1) Radio spectral index variations of the SNR HB3 (2) Radio spectral index study of the SNRs OA184 and VRO42.05.01
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
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
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