Issue |
A&A
Volume 520, September-October 2010
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 2 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/200913670e | |
Published online | 07 October 2010 |
A scenario of planet erosion by coronal radiation (Corrigendum)*
1
Laboratorio de Astrofísica Estelar y Exoplanetas,
Centro de Astrobiología / CSIC-INTA, LAEFF Campus, PO Box 78,
28691 Villanueva de la Cañada, Madrid, Spain e-mail: jsanz@cab.inta-csic.es
2
Institut de Ciènces de l'Espai (CSIC-IEEC), Campus UAB, Fac.
de Ciències, Torre C5-parell-2a planta,
08193 Bellaterra, Spain
3
INAF – Osservatorio Astronomico di Palermo
G. S. Vaiana, Piazza del Parlamento 1, 90134 Palermo, Italy
4
SOC, European Space Agency, ESAC, Apartado 78,
28691 Villanueva de la Cañada, Madrid, Spain
5
Instituto de Astrofísica de Canarias, 38205 La Laguna, Spain
6
Grantecan CALP, 38712 Breña Baja, La Palma, Spain
7
Spanish Virtual Observatory, Centro de Astrobiología /
CSIC-INTA, LAEFF Campus, Madrid, Spain
8
Dpto. de Física Teórica, C-XI, Facultad de Ciencias,
Universidad Autónoma de Madrid, Cantoblanco, 28049 Madrid, Spain
In the notes to Table 1, a unit
conversion was incorrect. The text should read 1 MJ Gyr-1 = 6.02e+13 g s-1. As a consequence in the 3rd paragraph of Sect. 3, the mass loss taking place in
τ Boo b should be
= 0.011 MJ Gyr-1 for
ρ = 1 g cm-3, or
= 3.4
Gyr-1 in Earth mass units.
Independently, the values of “
accumulated”, in Col. 12 of Table 1 were calculated using an obsolete formula and were
thus slightly underestimated, generally by
0.2.
As a consequence Fig. 2 should show all values at a
slightly higher position, although this is of no relevance for the
conclusions of the paper. Table 1 and Fig. 2 are reproduced in
their correct version here. At the end of 5th paragraph of Sect. 2, the hard limit of
X-ray flux accumulated after 10 Gyr should be ~1022.14 erg cm-2, instead of ~1021.76 erg cm-2, and our
highest flux is now 1021.23 erg cm-2 instead of 1021.05 erg cm-2.
Key words: planetary systems / stars: coronae / astrobiology / X-rays: stars / errata, addenda
Table 1 is only available in electronic form at http://www.aanda.org
© ESO, 2010
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