activity
20072026
most citedRadio to gamma-ray variability study of blazar S5 0716+714

116 citations · 1.6k across the 50 of their papers we have counts for

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Showing 2017Show all

5 papers · 1 filter

astro-ph.GA2017★ 12 cited

Clues to NaCN formation

G. Quintana-Lacaci, J. Cernicharo, L. Velilla Prieto +5

ALMA is providing us essential information on where certain molecules form. Observing where these molecules emission arises from, the physical conditions of the gas, and how this r…

astro-ph.SR2017★ 52 cited

The Abundance of SiC2 in Carbon Star Envelopes: Evidence that SiC2 is a gas-phase precursor of SiC dust

S. Massalkhi, M. Agúndez, J. Cernicharo +6

Silicon carbide dust is ubiquitous in circumstellar envelopes around C-rich AGB stars. However, the main gas-phase precursors leading to the formation of SiC dust have not yet been…

astro-ph.SR2017★ 21 cited

The circumstellar envelope around the S-type AGB star W Aql Effects of an eccentric binary orbit

S. Ramstedt, S. Mohamed, W. H. T. Vlemmings +9

The CO(J=3-2) emission from the CSE of the binary S-type AGB star W Aql has been observed at subarcsecond resolution using ALMA. The aim of this paper is to investigate the wind pr…

astro-ph.GA2017★ 53 cited

IRC +10 216 in 3-D: morphology of a TP-AGB star envelope

M. Guélin, N. A. Patel, M. Bremer +10

During their late pulsating phase, AGB stars expel most of their mass in the form of massive dusty envelopes, an event that largely controls the composition of interstellar matter.…

astro-ph.SR2017★ 91 cited

The growth of carbon chains in IRC+10216 mapped with ALMA

M. Agundez, J. Cernicharo, G. Quintana-Lacaci +9

Linear carbon chains are common in various types of astronomical molecular sources. Possible formation mechanisms involve both bottom-up and top-down routes. We have carried out a…