output
20052026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2015 · astro-ph.SRShow all

23 papers · 2 filters

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.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.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.…

astro-ph.SR2015★ 106 cited

Episodic molecular outflow in the very young protostellar cluster Serpens South

Adele L. Plunkett, Hector G. Arce, Diego Mardones +5

The loss of mass from protostars, in the form of a jet or outflow, is a necessary counterpart to protostellar mass accretion. Outflow ejection events probably vary in their velocit…

astro-ph.SR2015★ 28 cited

From forced collapse to H ii region expansion in Mon R2: Envelope density structure and age determination with Herschel

P. Didelon, F. Motte, P. Tremblin +32

The surroundings of HII regions can have a profound influence on their development, morphology, and evolution. This paper explores the effect of the environment on H II regions in…

astro-ph.SR2015

SOFIA/FORCAST Observations of Warm Dust in S106: A Fragmented Environment

J. D. Adams, T. L. Herter, J. L. Hora +22

We present mid-IR (19 - 37 microns) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6 - 8.0 microns), IRTF/MIRLIN (11.3 and…