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

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Showing 2013Show all

7 papers · 1 filter

astro-ph.GA2013★ 229 cited

From Filamentary Networks to Dense Cores in Molecular Clouds: Toward a New Paradigm for Star Formation

Philippe André, James Di Francesco, Derek Ward-Thompson +3

Recent studies of the nearest star-forming clouds of the Galaxy at submillimeter wavelengths with the Herschel Space Observatory have provided us with unprecedented images of the i…

astro-ph.CO2013

Detection of the tSZ effect with the NIKA camera

B. Comis, R. Adam, J. F. Macías-Pérez +35

We present the first detection of the thermal Sunyaev-Zel'dovich (tSZ) effect from a cluster of galaxies performed with a KIDs (Kinetic Inductance Detectors) based instrument. The…

astro-ph.GA2013★ 233 cited

SDC13 infrared dark clouds: Longitudinally collapsing filaments?

N. Peretto, G. A. Fuller, Ph. André +11

Formation of stars is now believed to be tightly linked to the dynamical evolution of interstellar filaments in which they form. In this paper we analyze the density structure and…

astro-ph.GA2013★ 84 cited

Ion-neutral friction and accretion-driven turbulence in self-gravitating filaments

Patrick Hennebelle, Philippe André

Recent Herschel observations have confirmed that filaments are ubiquitous in molecular clouds and suggest that irrespectively of the column density, there is a characteristic width…

astro-ph.GA2013★ 27 cited

Herschel survey of brown dwarf disks in Rho Ophiuchi

C. Alves de Oliveira, P. Ábrahám, G. Marton +6

Recent observations of the Rho Ophiuchi cluster with the Herschel Space Observatory allow us to probe the spectral energy distribution (SED) of the brown dwarf population in the fa…

astro-ph.EP2013★ 17 cited

Identification of transitional disks in Chamaeleon with Herschel

Á. Ribas, B. Merín, H. Bouy +11

Transitional disks are circumstellar disks with inner holes that in some cases are produced by planets and/or substellar companions in these systems. For this reason, these disks a…