Volume 451, Number 3, June I 2006
|Page(s)||991 - 991|
|Section||Interstellar and circumstellar matter|
|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
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.