activity
20022026
most citedThe Dynamics of Massive Starless Cores with ALMA

170 citations · 6.6k across the 187 of their papers we have counts for

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Showing 2012Show all

8 papers · 1 filter

astro-ph.GA2012★ 103 cited

Early stages of cluster formation: fragmentation of massive dense cores down to ~1000 AU

Aina Palau, Asunción Fuente, Josep M. Girart +11

In order to study the fragmentation of massive dense cores, which constitute the cluster cradles, we observed with the PdBI in the most extended configuration the continuum at 1.3…

astro-ph.GA2012★ 60 cited

Different evolutionary stages in massive star formation. Centimeter continuum and H2O maser emission with ATCA

A. Sanchez-Monge, M. T. Beltran, R. Cesaroni +5

We present ATCA observations of the H2O maser line and radio continuum at 18.0GHz and 22.8GHz, toward a sample of 192 massive star forming regions containing several clumps already…

astro-ph.SR2012★ 96 cited

Complex, Quiescent Kinematics in a Highly Filamentary Infrared Dark Cloud

Jonathan D. Henshaw, Paola Caselli, Francesco Fontani +3

Infrared Dark Clouds (IRDCs) host the initial conditions under which massive stars and stellar clusters form. We have obtained high sensitivity and high spectral resolution observa…

astro-ph.GA2012★ 39 cited

A Virialized Filamentary Infrared Dark Cloud

Audra K. Hernandez, Jonathan C. Tan, Jouni Kainulainen +4

The initial conditions of massive star and star cluster formation are expected to be cold, dense and high column density regions of the interstellar medium, which can reveal themse…

astro-ph.GA2012★ 10 cited

Close encounters of the protostellar kind in IC 1396N

M. T. Beltran, F. Massi, F. Fontani +2

We have mapped in the 2.7 mm continuum and 12CO with the PdBI the IR-dark "tail" that crosses the IC 1396N globule from south to north, and is the most extincted part of this cloud…

astro-ph.GA2012★ 67 cited

High CO depletion in southern infrared-dark clouds

F. Fontani, A. Giannetti, M. T. Beltran +5

Infrared-dark high-mass clumps are among the most promising objects to study the initial conditions of the formation process of high-mass stars and rich stellar clusters. In this w…