Volume 617, September 2018
|Number of page(s)||1|
|Section||Planets and planetary systems|
|Published online||25 September 2018|
Exploring the climate of Proxima B with the Met Office Unified Model (Corrigendum)
Physics and Astronomy, College of Engineering, Mathematics and Physical Sciences, University of Exeter, Exeter,
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.
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.
|Open with DEXTER|
© ESO 2018
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