output
20052026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2015Show all

76 papers · 1 filter

astro-ph.SR2015★ 39 cited

Implication of Formation Mechanisms of HC5N in TMC-1 as Studied by 13C Isotopic Fractionation

Kotomi Taniguchi, Hiroyuki Ozeki, Masao Saito +5

We observed the J = 9-8 and 16-15 rotational transitions of the normal species and five 13C isotopologues of HC5N to study its formation mechanisms toward the cyanopolyyne peak in…

astro-ph.GA2015★ 199 cited

A multi-wavelength analysis for interferometric (sub-)mm observations of protoplanetary disks: radial constraints on the dust properties and the disk structure

M. Tazzari, L. Testi, B. Ercolano +20

Theoretical models of grain growth predict dust properties to change as a function of protoplanetary disk radius, mass, age and other physical conditions. We lay down the methodolo…

astro-ph.GA2015★ 16 cited

Spatially-resolved Radio-to-Far-infrared SED of the Luminous Merger Remnant NGC 1614 with ALMA and VLA

Toshiki Saito, Daisuke Iono, Cong K. Xu +9

We present the results of Atacama Large Millimeter/Submillimeter Array (ALMA) 108, 233, 352, and 691 GHz continuum observations and Very Large Array (VLA) 4.81 and 8.36 GHz observa…

astro-ph.SR2015★ 53 cited

Two-level hierarchical fragmentation in the Orion Molecular Cloud 1 northern filament

P. S. Teixeira, S. Takahashi, L. A. Zapata +1

[Abridged] We have recently reported on the collapse and fragmentation properties of the northernmost part of this structure, located ~2.4pc north of Orion KL -- the Orion Molecula…

astro-ph.GA2015★ 75 cited

Submillimeter-HCN Diagram for an Energy Diagnostics in the Centers of Galaxies

Takuma Izumi, Kotaro Kohno, Susanne Aalto +16

Compiling data from literature and the ALMA archive, we show enhanced HCN(4-3)/HCO(4-3) and/or HCN(4-3)/CS(7-6) integrated intensity ratios in circumnuclear molecular gas aroun…

astro-ph.SR2015★ 10 cited

A submillimeter search for pre- and proto-brown dwarfs in Chamaeleon II

I. de Gregorio-Monsalvo, D. Barrado, H. Bouy +7

Context. Chamaeleon II molecular cloud is an active star forming region that offers an excellent opportunity for studying the formation of brown dwarfs in the southern hemisphere.…