activity
20062026
most citedA highly-collimated SiO jet in the HH212 protostellar outflow

109 citations · 769 across the 23 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2026

Evidence for a bloated massive protostar in IRAS20126+4104

Riccardo Cesaroni

Variability is a well known phenomenon in low-mass young stellar objects, but in recent years the monitoring of methanol masers and infrared continuum emission has permitted the de…

astro-ph.SR2025★ 4 cited

Protostellar Outflows at the EarliesT Stages (POETS) VI. Evidence of disk-wind in G11.92-0.61 MM1

O. S. Bayandina, L. Moscadelli, R. Cesaroni +3

Magnetohydrodynamic disk-winds play a key role in the formation of massive stars by providing the fine-tuning between accretion and ejection, where excess angular momentum is redir…

astro-ph.SR2024

Dissecting the disk and the jet of a massive (proto)star. An ALMA view of IRAS20126+4104

R. Cesaroni, D. Galli, M. Padovani +2

We investigate one of the best examples of disk+jet systems around an early B-type (proto)star, IRAS20126+4104. This object is an ideal target for resolution of its disk and the de…

astro-ph.SR2024

Radio outburst from a massive (proto)star. III. Unveiling the bipolarity of the radio jet from S255IR NIRS3

R. Cesaroni, L. Moscadelli, A. Caratti o Garatti +6

We report new Very Large Array high-resolution observations of the radio jet from the outbursting high-mass star S255IR~NIRS3. The images at 6, 10, and 22.2 GHz confirm the existen…

astro-ph.SR2019★ 79 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.SR2018★ 65 cited

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★ 64 cited

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-ph.SR2013★ 19 cited

A study on subarcsecond scales of the ammonia and continuum emission toward the G16.59-0.05 high-mass star-forming region

L. Moscadelli, R. Cesaroni, Á. Sánchez-Monge +4

We wish to investigate the structure, velocity field, and stellar content of the G16.59-0.05 high-mass star-forming region, where previous studies have established the presence of…

astro-ph.SR2010★ 102 cited

Methanol and water masers in IRAS 20126+4104: The distance, the disk, and the jet

L. Moscadelli, R. Cesaroni, M. J. Rioja +2

IRAS 20126+4104 is one of the best candidates for a high-mass (proto)star surrounded by an accretion disk. Such a fact may be used to set constraints on theories of high-mass star…