activity
20082025
most citedFirst detection of glycolaldehyde outside the Galactic Center

136 citations · 550 across the 10 of their papers we have counts for

collaborators

10 papers

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.SR2019★ 37 cited

Protostellar Outflows at the EarliesT Stages (POETS). II. A possible radio synchrotron jet associated with the EGO G035.02+0.35

A. Sanna, L. Moscadelli, C. Goddi +7

Centimeter continuum observations of protostellar jets have revealed the presence of knots of shocked gas where the flux density decreases with frequency. This spectrum is characte…

astro-ph.SR2016★ 48 cited

Binary system and jet precession and expansion in G35.20-0.74N

M. T. Beltrán, R. Cesaroni, L. Moscadelli +3

Context. ALMA observations of the high-mass star-forming region G35.20-0.74N have revealed the presence of a Keplerian disk in core B rotating about a massive object of 18 Msun, as…

astro-ph.GA2016★ 15 cited

Origin of the Lyman excess in early-type stars

R. Cesaroni, Á. Sánchez-Monge, M. T. Beltrán +3

Ionized regions around early-type stars are believed to be well-known objects, but until recently, our knowledge of the relation between the free-free radio emission and the IR emi…

astro-ph.GA2013★ 126 cited

A candidate circumbinary Keplerian disk in G35.20-0.74 N: A study with ALMA

A. Sanchez-Monge, R. Cesaroni, M. T. Beltran +13

We report on ALMA observations of continuum and molecular line emission with 0.4" resolution towards the high-mass star forming region G35.20-0.74 N. Two dense cores are detected i…

astro-ph.GA2012★ 67 cited

High CO depletion in southern infrared-dark clouds

F. Fontani, A. Giannetti, M. T. Beltran +5

Infrared-dark high-mass clumps are among the most promising objects to study the initial conditions of the formation process of high-mass stars and rich stellar clusters. In this w…