About: Mousis O.

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Attributs	Valeurs
type	Person
sameAs	Mousis O.
name	Mousis O. Mousis Olivier Mousis, Olivier Mousis, O.
personal mailbox	Olivier.Mousis@obs-besancon.fr
familyName	Mousis
Given name	O. Olivier
is relates of	http://hub.abes.fr/oup/periodical/mnrasl/2009/volume_397/issue_1/101111j17453933200900687x/authorship/3 http://hub.abes.fr/oup/periodical/mnrasl/2005/volume_362/issue_1/101111j17453933200500070x/authorship/1 http://hub.abes.fr/oup/periodical/mnras/2005/volume_358/issue_1/101111j13652966200508777x/authorship/1 http://hub.abes.fr/edp/periodical/aa/2023/volume_670/issue_2023/aa44670-22/authorship/2 http://hub.abes.fr/edp/periodical/aa/2023/volume_674/issue_2023/aa45961-23/authorship/24 http://hub.abes.fr/edp/periodical/aa/2022/volume_667/issue_2022/aa43775-22/authorship/4 http://hub.abes.fr/edp/periodical/aa/2023/volume_674/issue_2023/aa45660-22/authorship/35 http://hub.abes.fr/edp/periodical/aa/2023/volume_673/issue_2023/aa45741-22/authorship/26 http://hub.abes.fr/edp/periodical/aa/2023/volume_677/issue_2023/aa45736-22/authorship/3
is Author of	Can collisional activity produce a crystallization of Edgeworth-Kuiper Belt comets? Expectations for the Deep Impact collision from modelling of cometary nuclei On the composition of ices incorporated in Ceres Volatile-rich comets ejected early on during Solar System formation Evolution of the reservoirs of volatiles in the protosolar nebula The young mini-Neptune HD 207496b that is either a naked core or on the verge of becoming one Near-IR and optical radial velocities of the active M dwarf star Gl 388 (AD Leo) with SPIRou at CFHT and SOPHIE at OHP TOI-733 b: A planet in the small-planet radius valley orbiting a Sun-like star Interior-atmosphere modelling to assess the observability of rocky planets with JWST

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