activity
20062023
most citedATLASGAL --- properties of a complete sample of Galactic clumps

362 citations · 2k across the 41 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR201953 cited

Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core

C. Gieser, D. Semenov, H. Beuther +30

We present a detailed observational and modeling study of the hot core VLA 3 in the high-mass star-forming region AFGL 2591, which is a target region of the NOrthern Extended Milli…

astro-ph.SR2019

Fragmentation, rotation and outflows in the high-mass star-forming region IRAS 23033+5951. A case study of the IRAM NOEMA large program CORE

F. Bosco, H. Beuther, A. Ahmadi +23

The formation process of high-mass stars (>8M) is poorly constrained, particularly, the effects of clump fragmentation creating multiple systems and the mechanism of mass a…

astro-ph.SR201922 cited

IRAS23385+6053: An embedded massive cluster in the making

R. Cesaroni, H. Beuther, A. Ahmadi +26

This study is part of the project ``CORE'', an IRAM/NOEMA large program consisting of observations of the millimeter continuum and molecular line emission towards 20 selected high-…

astro-ph.SR201924 cited

First interferometric study of enhanced N-fractionation in NH: the high-mass star-forming region IRAS 05358+3543

L. Colzi, F. Fontani, P. Caselli +3

Nitrogen (N) fractionation is used as a tool to search for a link between the chemical history of the Solar System and star-forming regions. A large variation of N/N…

astro-ph.SR2018

Water and interstellar complex organics associated with the HH 212 protostellar disc - On disc atmospheres, disc winds, and accretion shocks

C. Codella, E. Bianchi, B. Tabone +14

The HH 212 protostellar system, in Orion B, has been mapped thanks to ALMA-Band 7 Cycle 1 and Cycle 4 observations of dueterated water (HDO) and acetaldehyde (CHCHO) emission w…

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…