activity
20092015
most cited[OI]63micron jets in class 0 sources detected by Herschel

67 citations · 503 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2015★ 63 cited

Jet multiplicity in the proto-binary system NGC1333-IRAS4A. The detailed CALYPSO IRAM-PdBI view

G. Santangelo, C. Codella, S. Cabrit +10

Owing to the paucity of sub-arcsecond (sub)mm observations required to probe the innermost regions of newly forming protostars, several fundamental questions are still being debate…

astro-ph.GA2015★ 26 cited

Disentangling the jet emission from protostellar systems. The ALMA view of VLA1623

G. Santangelo, N. M. Murillo, B. Nisini +4

Context: High-resolution studies of class 0 protostars represent the key to constraining protostar formation models. VLA16234-2417 represents the prototype of class 0 protostars, a…

astro-ph.SR2015★ 67 cited

[OI]63micron jets in class 0 sources detected by Herschel

B. Nisini, G. Santangelo, T. Giannini +9

We present Herschel PACS mapping observations of the [OI]63 micron line towards protostellar outflows in the L1448, NGC1333-IRAS4, HH46, BHR71 and VLA1623 star forming regions. We…

astro-ph.GA2014★ 3 cited

Resolving the shocked gas in HH54 with Herschel: CO line mapping at high spatial and spectral resolution

P. Bjerkeli, R. Liseau, C. Brinch +11

The HH54 shock is a Herbig-Haro object, located in the nearby Chamaeleon II cloud. Observed CO line profiles are due to a complex distribution in density, temperature, velocity, an…

astro-ph.SR2014★ 45 cited

Shockingly low water abundances in Herschel / PACS observations of low-mass protostars in Perseus

A. Karska, L. E. Kristensen, E. F. van Dishoeck +16

Protostars interact with their surroundings through jets and winds impacting on the envelope and creating shocks, but the nature of these shocks is still poorly understood. Our aim…

astro-ph.GA2014★ 15 cited

First spectrally-resolved H observations towards HH 54 / Low HO abundance in shocks

G. Santangelo, S. Antoniucci, B. Nisini +11

Context: Herschel observations suggest that the HO distribution in outflows from low-mass stars resembles the H emission. It is still unclear which of the different excitat…