100 citations · 596 across the 33 of their papers we have counts for
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3D radiative hydrodynamic simulations of protostellar collapse with H-C-O dynamical chemistry
Natalia Dzyurkevich, Benoît Commerçon, Pierre Lesaffre +1
Combining the co-evolving chemistry, hydrodynamics and radiative transfer is an important step for star formation studies. It allows both a better link to observations and a self-c…
Chemistry in Disks X: The Molecular Content of Proto-planetary Disks in Taurus
S. Guilloteau, L. Reboussin, A. Dutrey +6
(abridged) We used the IRAM 30-m to perform a sensitive wideband survey of 30 protoplanetary disks in the Taurus Auriga region. We simultaneously observed HCO(3-2), HCN(3-2), C…
Cold CO gas in the disk of the young eruptive star EX Lup
Ágnes Kóspál, Péter Ábrahám, Timea Csengeri +6
EX Lupi-type objects (EXors) form a sub-class of T Tauri stars, defined by sudden sporadic flare-ups of 1-5 magnitudes at optical wavelengths. These eruptions are attributed to enh…