Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1
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The habitability of the Milky Way during the active phase of its central supermassive black hole.Formation of TRAPPIST-1 and other compact systemsUV surface habitability of the TRAPPIST-1 systemExploring the climate of Proxima B with the Met Office Unified ModelHADES RV Programme with HARPS-N at TNG
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Water loss from terrestrial planets orbiting ultracool dwarfs: implications for the planets of TRAPPIST-1
description
im Oktober 2016 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в жовтні 2016
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name
Water loss from terrestrial pl ...... for the planets of TRAPPIST-1
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Water loss from terrestrial pl ...... for the planets of TRAPPIST-1
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type
label
Water loss from terrestrial pl ...... for the planets of TRAPPIST-1
@en
Water loss from terrestrial pl ...... for the planets of TRAPPIST-1
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prefLabel
Water loss from terrestrial pl ...... for the planets of TRAPPIST-1
@en
Water loss from terrestrial pl ...... for the planets of TRAPPIST-1
@nl
P2093
P2860
P356
P1476
Water loss from terrestrial pl ...... for the planets of TRAPPIST-1
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P2093
E. Bolmont
J. E. Owen
J. Leconte
S. N. Raymond
P2860
P304
P356
10.1093/MNRAS/STW2578
P407
P577
2016-10-08T00:00:00Z
P818
1605.00616
P819
2017MNRAS.464.3728B