| Issue |
A&A
Volume 532, August 2011
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 2 | |
| Section | Astrophysical processes | |
| DOI | https://doi.org/10.1051/0004-6361/201016364e | |
| Published online | 12 July 2011 | |
Corrigendum
The termination region of high-mass microquasar jets (corrigendum)
1 Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland
e-mail: valenti@cp.dias.ie
2 Dept. d’Astronomia i Astrofísica, Universitat de València, C/ Dr. Moliner 50, 46100, Burjassot (València), Spain
e-mail: Manel.Perucho@uv.es
3
Institut für Astronomie und Astrophysik, Universität Tübingen, Sand 1, 72076 Tübingen, Germany
4
INTEGRAL Science Data Centre, Université de Genève, Chemin d’Ecogia 16, 1290 Versoix, Switzerland
e-mail: pol.bordas@uni-tuebingen.de
Key words: X-rays: binaries / ISM: jets and outflows / radiation mechanisms: nonthermal / Errata, addenda
In the work by Bosch-Ramon et al. (2011), a mistake was made when preparing the setup of simulation 3, which corresponds to a microquasar jet launched when the binary proper motion has already affected the shape of the massive star wind-blown bubble (see Fig. 1, bottom, in Bosch-Ramon et al. 2011). We redid the simulation with the proper setup values, which are presented in Table 1. The new density, pressure, temperature, and axial velocity 2-dimensional maps are presented in Figs. 1 and 2. As can be seen when comparing these figures with Figs. 10 and 11
in Bosch-Ramon et al. (2011), the results are qualitatively the same, and therefore conclusions remain unchanged. In case the proper motion has already distorted the stellar wind-blown bubble, the jet will be completely destroyed before reaching the unshocked ISM.
The ambient medium in case 3.
 |
Fig. 1 Maps of density (top) and pressure (bottom) at the last snapshot of the simulation (tsrc ≈ 340 yr). The shocked wind moves from top to bottom. |
 |
Fig. 2 Maps of temperature (top) and axial velocity (bottom) at the last snapshot of the simulation (tsrc ≈ 340 yr). The shocked wind moves from top to bottom. |
References
- Bosch-Ramon, V., Perucho, M., & Bordas, P. 2011, A&A, 528, A89 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO, 2011
All Tables
All Figures
|
Fig. 1 Maps of density (top) and pressure (bottom) at the last snapshot of the simulation (tsrc ≈ 340 yr). The shocked wind moves from top to bottom. |
| In the text | |
|
Fig. 2 Maps of temperature (top) and axial velocity (bottom) at the last snapshot of the simulation (tsrc ≈ 340 yr). The shocked wind moves from top to bottom. |
| In the text | |
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