262 citations · 5.7k across the 111 of their papers we have counts for
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AB Aur, a Rosetta stone for studies of planet formation (II): HS detection and sulfur budget
Pablo Rivière-Marichalar, Asunción Fuente, Gisela Esplugues +7
The sulfur abundance is poorly known in most environments. Yet, deriving the sulfur abundance is key to understanding the evolution of the chemistry from molecular clouds to planet…
Gas phase Elemental abundances in Molecular cloudS (GEMS) VI. A sulphur journey across star-forming regions: study of thioformaldehyde emission
G. Esplugues, A. Fuente, D. Navarro-Almaida +10
In the context of the IRAM 30m Large Program GEMS, we present a study of thioformaldehyde in several starless cores located in star-forming filaments of Taurus, Perseus, and Orion.…
HS observations in young stellar disks in Taurus
P. Rivière-Marichalar, A. Fuente, R. Le Gal +7
Context. Studying gas chemistry in protoplanetary disks is key to understanding the process of planet formation. Sulfur chemistry in particular is poorly understood in interstellar…
Gas kinematics of key prebiotic molecules in GV Tau N revealed with an ALMA, PdBI, and Herschel synergy
A. Fuente, S. P. Treviño-Morales, R. Le Gal +4
A large effort has been made to detect warm gas in the planet formation zone of circumstellar discs using space and ground-based near infrared facilities. GV Tau N, the most obscur…
Gas accretion within the dust cavity in AB Aur
Pablo Rivière-Marichalar, Asuncioón Fuente, Clément Baruteau +5
AB Aur is a Herbig Ae star hosting a well-known transitional disk. Because of its proximity and low inclination angle, it is an excellent object to study planet formation. Our goal…
Evidence for disks at an early stage in class 0 protostars?
M. Gerin, J. Pety, B. Commercon +8
The formation epoch of protostellar disks is debated because of the competing roles of rotation, turbulence, and magnetic fields in the early stages of low-mass star formation. Mag…