| Issue |
A&A
Volume 617, September 2018
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/201630020e | |
| Published online | 25 September 2018 | |
Exploring the climate of Proxima B with the Met Office Unified Model (Corrigendum)
1
Physics and Astronomy, College of Engineering, Mathematics and Physical Sciences, University of Exeter, Exeter,
EX4 4QL,
UK
e-mail: i.boutle@exeter.ac.uk
2
Met Office,
FitzRoy Road, Exeter, EX1 3PB,
UK
3
Mathematics, College of Engineering, Mathematics and Physical Sciences, University of Exeter, Exeter,
EX4 4QF,
UK
Key words: stars: individual: Proxima Cen / planets and satellites: individual: Proxima B / planets and satellites: atmospheres / planets and satellites: detection / planets and satellites: terrestrial planets / errata, addenda
It has been brought to our attention that there is a minor typo in the x-axis title of the second panel of Fig. 5, which should have units of “kg kg−1” rather than “g kg−1”. The corrected figure appears below.
 |
Fig. 5 Ten orbit mean profiles of temperature and water vapour (left and right panels, respectively) from the sub-stellar point on the dayside of the tidally locked planet (solid) and its antipode (dashed). Filled triangles show the surface temperature, and crosses indicate the position of the model levels. |
© ESO 2018
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