167 citations · 5.3k across the 151 of their papers we have counts for
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Hot methanol from the inner region of the HH 212 protostellar system
S. Leurini, C. Codella, S. Cabrit +9
The mechanisms leading to the formation of disks around young stellar objects (YSOs) and to the launching of the associated jets are crucial to the understanding of the earliest st…
The 2008 outburst in the Young Stellar System Z CMa. III - Multi-epoch high-angular resolution images and spectra of the components in near-infrared
M. Bonnefoy, G. Chauvin, C. Dougados +8
Z CMa is a complex pre-main sequence binary with a current separation of 100 mas, known to consist of an FU Orionis star (SE component) and an embedded Herbig Be star (NW component…
Sub-0.1" optical imaging of the Z CMa jets with SPHERE/ZIMPOL
S. Antoniucci, L. Podio, B. Nisini +15
Crucial information on the mass accretion-ejection in young stars can be obtained from high spatial resolution images of jets in sources with recurrent accretion outbursts. Using t…
First image of the L1157 molecular jet by the CALYPSO IRAM-PdBI survey
L. Podio, C. Codella, F. Gueth +12
Fast jets are thought to be a crucial ingredient of star formation because they might extract angular momentum from the disk and thus allow mass accretion onto the star. However, i…
The small-scale HH34 IRS jet as seen by X-shooter
B. Nisini, T. Giannini, S. Antoniucci +3
Very little information has been so far gathered on atomic jets from young embedded low mass sources (class I stars), especially in the inner jet region. We exploit multiwave spect…
H2S in the L1157-B1 Bow shock
Jonathan Holdship, Serena Viti, Izaskun Jimenez-Serra +8
Sulfur-bearing molecules are highly reactive in the gas phase of the ISM. However, the form in which most of the sulfur is locked onto interstellar dust grains is unknown. By takin…