activity
20092021
most citedCluster-formation in the Rosette molecular cloud at the junctions of filaments

358 citations · 5.5k across the 82 of their papers we have counts for

collaborators

83 papers

astro-ph.GA2021★ 22 cited

Probing the structure of a massive filament: ArTeMiS 350 and 450 micron mapping of the integral-shaped filament in Orion A

F. Schuller, Ph. André, Y. Shimajiri +18

(abridged) Within the Orion A molecular cloud, the integral-shaped filament (ISF) is a prominent, degree-long structure of dense gas and dust, with clear signs of recent and on-goi…

astro-ph.GA2021★ 36 cited

Revealing the diverse magnetic field morphologies in Taurus dense cores with sensitive sub-millimeter polarimetry

Chakali Eswaraiah, Di Li, Ray S. Furuya +142

We have obtained sensitive dust continuum polarization observations at 850 m in the B213 region of Taurus using POL-2 on SCUBA-2 at the James Clerk Maxwell Telescope (JCMT), as…

astro-ph.GA2021★ 24 cited

GASTON: Galactic Star Formation with NIKA2. Evidence for the mass growth of star-forming clumps

A. J. Rigby, N. Peretto, R. Adam +44

Determining the mechanism by which high-mass stars are formed is essential for our understanding of the energy budget and chemical evolution of galaxies. By using the New IRAM KIDs…

astro-ph.SR2021★ 85 cited

The CALYPSO IRAM-PdBI survey of jets from Class 0 protostars. Are jets ubiquitous in young stars ?

L. Podio, B. Tabone, C. Codella +10

As a part of the CALYPSO large programme, we constrain the properties of protostellar jets and outflows in a sample of 21 Class 0 protostars with internal luminosities, Lint, from…

astro-ph.SR2020★ 5 cited

Probing episodic accretion with chemistry: CALYPSO observations of IRAM 04191+1522. Results from the CALYPSO IRAM-PdBI survey

S. Anderl, S. Maret, S. Cabrit +7

Context. The process of mass accretion in the earliest phases of star formation is still not fully understood: Does the accretion rate smoothly decline with the age of the protosta…

astro-ph.GA2020★ 39 cited

Mass segregation and sequential star formation in NGC 2264 revealed by Herschel

T. Nony, J. -F. Robitaille, F. Motte +16

The mass segregation of stellar clusters could be primordial rather than dynamical. Despite the abundance of studies of mass segregation for stellar clusters, those for stellar pro…