activity
20072022
most citedCould we identify hot Ocean-Planets with CoRoT, Kepler and Doppler velocimetry?

103 citations · 593 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2022★ 19 cited

ALMA-IMF IV -- A comparative study of the main hot cores in W43-MM1: detection, temperature and molecular composition

N. Brouillet, D. Despois, J. Molet +21

W43-MM1 is a young region, very rich in terms of high-mass star formation. We aim to systematically identify the massive cores which contain a hot core and compare their molecular…

astro-ph.GA2019★ 32 cited

Molecular analysis of a high-mass prestellar core candidate in W43-MM1

J. Molet, N. Brouillet, T. Nony +6

High-mass analogues of low-mass prestellar cores are searched for to constrain the models of high-mass star formation. Several high-mass cores, at various evolutionary stages, have…

astro-ph.GA2018★ 47 cited

Detection of a high-mass prestellar core candidate in W43-MM1

T. Nony, F. Louvet, F. Motte +11

Aims. To constrain the physical processes that lead to the birth of high-mass stars it is mandatory to study the very first stages of their formation. We search for high-mass analo…

astro-ph.SR2016★ 24 cited

Proper motion survey and kinematic analysis of the Rho Ophiuchi embedded cluster

C. Ducourant, R. Teixeira, A. Krone-Martins +7

We aim at performing a kinematic census of young stellar objects (YSOs) in the Rho Ophiuchi F core and partially in the E core of the L1688 dark cloud. We run a proper motion progr…

astro-ph.EP2015

Ethyl alcohol and sugar in comet C/2014Q2 (Lovejoy)

Nicolas Biver, Dominique Bockelée-Morvan, Raphaël Moreno +7

The presence of numerous complex organic molecules (COMs; defined as those containing six or more atoms) around protostars shows that star formation is accompanied by an increase o…

astro-ph.GA2015★ 63 cited

Antifreeze in the hot core of Orion - First detection of ethylene glycol in Orion-KL

N. Brouillet, D. Despois, X. -H. Lu +5

Comparison of their chemical compositions shows, to first order, a good agreement between the cometary and interstellar abundances. However, a complex O-bearing organic molecule, e…