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20112023
most citedCluster-formation in the Rosette molecular cloud at the junctions of filaments

358 citations · 2k across the 27 of their papers we have counts for

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19 papers · 1 filter

astro-ph.GA2022★ 12 cited

Gas kinematics around filamentary structures in the Orion B cloud

Mathilde Gaudel, Jan H. Orkisz, Maryvonne Gerin +27

Understanding the initial properties of star-forming material and how they affect the star formation process is key. From an observational point of view, the feedback from young hi…

astro-ph.GA2019★ 118 cited

Dynamics of cluster-forming hub-filament systems: The case of the high-mass star-forming complex Monoceros R2

S. P. Trevino-Morales, A. Fuente, A. Sanchez-Monge +15

High-mass stars and star clusters commonly form within hub-filament systems. Monoceros R2, harbors one of the closest such systems, making it an excellent target for case studies.…

astro-ph.GA2019★ 20 cited

The Origin of [CII] 158um Emission toward the HII Region Complex S235

L. D. Anderson, Z. Makai, M. Luisi +9

Although the 2P3/2-2P1/2 transition of [CII] at 158um is known to be an excellent tracer of active star formation, we still do not have a complete understanding of where within sta…

astro-ph.GA2017★ 37 cited

Clustering the Orion B giant molecular cloud based on its molecular emission

Emeric Bron, Chloé Daudon, Jérôme Pety +12

Previous attempts at segmenting molecular line maps of molecular clouds have focused on using position-position-velocity data cubes of a single line to separate the spatial compone…

astro-ph.GA2017★ 36 cited

Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane

P. Palmeirim, A. Zavagno, D. Elia +35

We present a comprehensive statistical analysis of star-forming objects located in the vicinities of 1 360 bubble structures throughout the Galactic Plane and their local environme…

astro-ph.GA2017★ 53 cited

Dissecting the molecular structure of the Orion B cloud: Insight from Principal Component Analysis

Pierre Gratier, Emeric Bron, Maryvonne Gerin +12

Context. The combination of wideband receivers and spectrometers currently available in (sub-)millimeter observatories deliver wide- field hyperspectral imaging of the interstellar…

astro-ph.GA2017★ 105 cited

Turbulence and star formation efficiency in molecular clouds: solenoidal versus compressive motions in Orion B

Jan H. Orkisz, Jérôme Pety, Maryvonne Gerin +13

The nature of turbulence in molecular clouds is one of the key parameters that control star formation efficiency: compressive motions, as opposed to solenoidal motions, can trigger…

astro-ph.GA2016★ 93 cited

Feedback in Clouds II: UV Photoionisation and the first supernova in a massive cloud

Sam Geen, Patrick Hennebelle, Pascal Tremblin +1

Molecular cloud structure is regulated by stellar feedback in various forms. Two of the most important feedback processes are UV photoionisation and supernovae from massive stars.…

astro-ph.GA2016★ 19 cited

Globules and Pillars in Cygnus X I. Herschel Far-infrared imaging of the Cyg OB2 environment

N. Schneider, S. Bontemps, F. Motte +21

The radiative feedback of massive stars on molecular clouds creates pillars, globules and other features at the interface between the HII region and molecular cloud. We present her…

astro-ph.GA2015★ 77 cited

Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X

N. Schneider, S. Bontemps, F. Motte +11

Column density (N) PDFs serve as a powerful tool to characterize the physical processes that influence the structure of molecular clouds. Star-forming clouds can best be characteri…

astro-ph.GA2015★ 97 cited

Detection of two power-law tails in the probability distribution functions of massive GMCs

N. Schneider, S. Bontemps, P. Girichidis +20

We report the novel detection of complex high-column density tails in the probability distribution functions (PDFs) for three high-mass star-forming regions (CepOB3, MonR2, NGC6334…

astro-ph.GA2015★ 41 cited

Filaments in the Lupus molecular clouds

M. Benedettini, E. Schisano, S. Pezzuto +19

We have studied the filaments extracted from the column density maps of the nearby Lupus 1, 3, and 4 molecular clouds, derived from photometric maps observed with the Herschel sate…

astro-ph.GA2015★ 83 cited

Photoionisation Feedback in a Self-Gravitating, Magnetised, Turbulent Cloud

Sam Geen, Patrick Hennebelle, Pascal Tremblin +1

We present a new set of analytic models for the expansion of HII regions powered by UV photoionisation from massive stars and compare them to a new suite of radiative magnetohydrod…

astro-ph.GA2014★ 87 cited

Understanding star formation in molecular clouds II. Signatures of gravitational collapse of IRDCs

N. Schneider, T. Csengeri, R. S. Klessen +6

We analyse column density and temperature maps derived from Herschel dust continuum observations of a sample of massive infrared dark clouds (G11.11-0.12, G18.82-0.28, G28.37+0.07,…

astro-ph.GA2014★ 125 cited

Understanding star formation in molecular clouds I. Effects of line-of-sight contamination on the column density structure

N. Schneider, V. Ossenkopf, T. Csengeri +6

Column-density maps of molecular clouds are one of the most important observables in the context of molecular cloud- and star-formation (SF) studies. With the Herschel satellite it…

astro-ph.GA2014★ 97 cited

Ionization compression impact on dense gas distribution and star formation, Probability density functions around H ii regions as seen by Herschel

P. Tremblin, N. Schneider, V. Minier +22

Ionization feedback should impact the probability distribution function (PDF) of the column density around the ionized gas. We aim to quantify this effect and discuss its potential…

astro-ph.GA2013★ 51 cited

Pillars and globules at the edges of H ii regions, Confronting Herschel observations and numerical simulations

P. Tremblin, V. Minier, N. Schneider +24

Pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M16) and the Rosette molecular cloud, and understanding their origin will help ch…

astro-ph.GA2012★ 45 cited

Globules and pillars seen in the [CII] 158 micron line with SOFIA

N. Schneider, R. Güsten, P. Tremblin +22

Molecular globules and pillars are spectacular features, found only in the interface region between a molecular cloud and an HII-region. Impacting Far-ultraviolet (FUV) radiation c…

astro-ph.GA2012★ 358 cited

Cluster-formation in the Rosette molecular cloud at the junctions of filaments

N. Schneider, T. Csengeri, M. Hennemann +31

For many years feedback processes generated by OB-stars in molecular clouds, including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to trigger su…