65 citations · 587 across the 19 of their papers we have counts for
19 papers
The role of low-mass star clusters in massive star formation in Orion
V. M. Rivilla, J. Martin-Pintado, I. Jimenez-Serra +1
To distinguish between the different theories proposed to explain massive star formation, it is crucial to establish the distribution, the extinction, and the density of low-mass s…
X-ray embedded stars as driving sources of outflow-driven turbulence in OMC1-S
V. M. Rivilla, J. Martin-Pintado, J. Sanz-Forcada +2
Outflows arising from very young stars affect their surroundings and influence the star formation in the parental core. Multiple molecular outflows and Herbig-Haro (HH) objects hav…
The role of low-mass star clusters in massive star formation. The Orion Case
V. M. Rivilla, J. Martin-Pintado, I. Jimenez-Serra +1
To distinguish between the different theories proposed to explain massive star formation, it is crucial to establish the distribution, the extinction, and the density of low-mass s…
Variability of the SiO thermal line emission toward the young L1448-mm outflow
I. Jimenez-Serra, J. Martin-Pintado, J. M. Winters +2
The detection of narrow SiO thermal emission toward young outflows has been proposed to be a signature of the magnetic precursor of C-shocks. Recent modeling of the SiO emission ac…
Unveiling the main heating sources in the Cepheus A HW2 region
I. Jimenez-Serra, J. Martin-Pintado, P. Caselli +4
We present high angular resolution PdBI images (beam of ~0.33'') of the J=27-26 line from several vibrational levels (v7=1 and v6=1) of HC3N toward Cepheus A HW2. These images reve…
On the evolution of the molecular line profiles induced by the propagation of C-shock waves
I. Jimenez-Serra, J. Martin-Pintado, P. Caselli +2
We present the first results of the expected variations of the molecular line emission arising from material recently affected by C-shocks (shock precursors). Our parametric model…