activity
20172022
most citedSeeds Of Life In Space (SOLIS): The organic composition diversity at 300--1000 au scale in Solar-type star forming regions

155 citations · 829 across the 17 of their papers we have counts for

collaborators

28 papers

astro-ph.GA202232 cited

FAUST III. Misaligned rotations of the envelope, outflow, and disks in the multiple protostellar system of VLA 16232417

Satoshi Ohashi, Claudio Codella, Nami Sakai +69

We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using HCO (), CS (), and CCH () lines as…

astro-ph.GA202235 cited

Ionised Gas Kinematics in MaNGA AGN. Extents of the Narrow Line and Kinematically Disturbed regions

A. Deconto-Machado, R. A. Riffel, G. S. Ilha +11

We analyse the kinematics of 170 AGN host galaxies as compared to those of a matched control sample of non-active galaxies from the MaNGA survey in order to characterise and estima…

astro-ph.GA2021

Fragmentation and kinematics in high-mass star formation: CORE-extension targeting two very young high-mass star-forming regions

H. Beuther, C. Gieser, S. Suri +24

Context: The formation of high-mass star-forming regions from their parental gas cloud and the subsequent fragmentation processes lie at the heart of star formation research. Aims:…

astro-ph.GA2021

A Low-mass Cold and Quiescent Core Population in a Massive Star Protocluster

Shanghuo Li, Xing Lu, Qizhou Zhang +24

Pre-stellar cores represent the initial conditions of star formation. Although these initial conditions in nearby low-mass star-forming regions have been investigated in detail, su…

astro-ph.GA202138 cited

ALMA-IRDC: Dense gas mass distribution from cloud to core scales

A. T. Barnes, J. D. Henshaw, F. Fontani +15

Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high-mass star formation (HMSF). Here we conduct an in-depth analysis of the fragmentation propertie…

astro-ph.GA20217 cited

The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"

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

We use sub-arcsecond resolution (0.4) observations with NOEMA at 1.37 mm to study the dust emission and molecular gas of 18 high-mass star-forming regions. We combine the…