L Velilla Prieto
Overview
Explore the profile of L Velilla Prieto including associated specialties, affiliations and a list of published articles.
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Snapshot
Articles
17
Citations
118
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0
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Recent Articles
1.
Sanchez Contreras C, Alcolea J, Bujarrabal V, Castro-Carrizo A, Prieto L, Santander-Garcia M, et al.
Astron Astrophys
. 2018 Nov;
618.
PMID: 30473586
We present continuum and molecular line emission ALMA observations of OH 231.8+4.2, a well studied bipolar nebula around an asymptotic giant branch (AGB) star. The high angular resolution and sensitivity...
2.
Cernicharo J, Guelin M, Agundez M, Pardo J, Massalkhi S, Fonfria J, et al.
Astron Astrophys
. 2018 Nov;
618.
PMID: 30429616
This work presents a detailed analysis of the laboratory and astrophysical spectral data available for SiC, SiC,SiC, SiCC, and SiC. New data on the rotational lines of these species between...
3.
Pardo J, Cernicharo J, Prieto L, Fonfria J, Agundez M, Quintana-Lacaci G, et al.
Astron Astrophys
. 2018 Sep;
615.
PMID: 30185989
Context: The variability in IRC+10216, the envelope of the asymptotic giant branch (AGB) star CW Leo, has attracted increasing attention in recent years. Studying the details of this variability in...
4.
Fonfria J, Fernandez-Lopez M, Pardo J, Agundez M, Sanchez Contreras C, Prieto L, et al.
Astrophys J
. 2018 Jul;
860(2).
PMID: 29977091
We present new high angular resolution interferometer observations of the = 0 = 14 - 13 and 15 - 14 SiS lines towards IRC+10216, carried out with CARMA and ALMA....
5.
Massalkhi S, Agundez M, Cernicharo J, Prieto L, Goicoechea J, Quintana-Lacaci G, et al.
Astron Astrophys
. 2018 Apr;
611.
PMID: 29628518
Context: 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 identified....
6.
Guelin M, Patel N, Bremer M, Cernicharo J, Castro-Carrizo A, Pety J, et al.
Astron Astrophys
. 2018 Feb;
610.
PMID: 29456257
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. The...
7.
Quintana-Lacaci G, Cernicharo J, Prieto L, Agundez M, Castro-Carrizo A, Fonfria J, et al.
Astron Astrophys
. 2017 Nov;
607.
PMID: 29151609
Context: 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 relates with...
8.
Cernicharo J, Agundez M, Prieto L, Guelin M, Pardo J, Kahane C, et al.
Astron Astrophys
. 2017 Nov;
606.
PMID: 29142328
We report the discovery in space of methyl silane, CHSiH, from observations of ten rotational transitions between 80 and 350 GHz ( from 4 to 16) with the IRAM 30...
9.
Agundez M, Cernicharo J, Quintana-Lacaci G, Castro-Carrizo A, Prieto L, Marcelino N, et al.
Astron Astrophys
. 2017 May;
601.
PMID: 28469283
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 combined observational and modeling...
10.
Prieto L, Sanchez Contreras C, Cernicharo J, Agundez M, Quintana-Lacaci G, Bujarrabal V, et al.
Astron Astrophys
. 2016 Dec;
597.
PMID: 28008187
Aims: We aim to investigate the physical and chemical properties of the molecular envelope of the oxygen-rich AGB star IK Tau. Methods: We carried out a millimeter wavelength line survey...