activity
20062019
most citedA highly-collimated SiO jet in the HH212 protostellar outflow

109 citations · 188 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.SR201979 cited

Substructures in the Keplerian disc around the O-type (proto)star G17.64+0.16

L. T. Maud, R. Cesaroni, M. S. N. Kumar +20

We present the highest angular resolution (20x15mas - 44x33au) Atacama Large Millimeter/sub-millimeter Array (ALMA) observations currently possible of the proto-O-star G17.64+0.16…

astro-ph.GA2018

Core fragmentation and Toomre stability analysis of W3(H2O): A case study of the IRAM NOEMA large program CORE

A. Ahmadi, H. Beuther, J. C. Mottram +30

The fragmentation mode of high-mass molecular clumps and the properties of the central rotating structures surrounding the most luminous objects have yet to be comprehensively char…

astro-ph.SR2018

Discovery of a sub-Keplerian disk with jet around a 20Msun young star. ALMA observations of G023.01-00.41

A. Sanna, A. Koelligan, L. Moscadelli +9

It is well established that Solar-mass stars gain mass via disk accretion, until the mass reservoir of the disk is exhausted and dispersed, or condenses into planetesimals. Accreti…

astro-ph.SR2018

Radio outburst from a massive (proto)star. When accretion turns into ejection

R. Cesaroni, L. Moscadelli, R. Neri +6

Context. Recent observations of the massive young stellar object S255 NIRS 3 have revealed a large increase in both methanol maser flux density and IR emission, which have been int…

astro-ph2006109 cited

A highly-collimated SiO jet in the HH212 protostellar outflow

C. Codella, S. Cabrit, F. Gueth +4

We mapped the HH212 Class 0 outflow in SiO(2--1, 5--4) and continuum using the PdBI in its extended configurations. The unprecedented angular resolution (down to 0.34") allows accu…