Issue |
A&A
Volume 565, May 2014
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/20030451e | |
Published online | 05 May 2014 |
Highly ionized Fe Kα emission lines from the LINER galaxy M 81 (Corrigendum)
Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey RH5 6NT, UK
e-mail: mjp@mssl.ucl.ac.uk
Key words: galaxies: individual: M81 (= NGC 3031) / galaxies: nuclei / galaxies: Seyfert / galaxies: active / X-rays: galaxies / errata, addenda
The exponent of the units on the y-axis of Fig. 4 is incorrect. A corrected version of the figure is presented here.
![]() |
Fig. 4 Confidence intervals for the energies and normalisations of the three narrow emission lines used to fit the bump between 6.25 and 7.15 keV. The solid, dashed, and dotted contours correspond to 1, 2, and 3σ confidence for two interesting parameters, respectively. The solid vertical lines indicate the expected energy for Fe I, Fe XXV, and Fe XXVI. |
Acknowledgments
We thank Andrew Young for bringing this mistake to our attention.
© ESO, 2014
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.