Luis Velilla Prieto

Showing 11 publications

2022

First detection of AIF line emission towards M-type AGB stars

M. Saberi, Theo Khouri, Luis Velilla Prieto et al
Astronomy and Astrophysics. Vol. 663
Journal article
2022

First detection of AlF line emission towards M-type AGB stars

M. Saberi, Theo Khouri, Luis Velilla Prieto et al
Astronomy and Astrophysics. Vol. 663
Journal article
2020

Detection of vibrationally excited HC7N and HC9N in IRC+10216

J. R. Pardo, C. Bermudez, C. Cabezas et al
Astronomy and Astrophysics. Vol. 640
Journal article
2020

The abundance of S- and Si-bearing molecules in O-rich circumstellar envelopes of AGB stars

S. Massalkhi, M. Agundez, J. Cernicharo et al
Astronomy and Astrophysics. Vol. 641
Journal article
2019

Detection of highly excited OH towards AGB stars: A new probe of shocked gas in the extended atmospheres

Theo Khouri, Luis Velilla Prieto, Elvire De Beck et al
Astronomy and Astrophysics. Vol. 623
Journal article
2019

Gas infall and possible circumstellar rotation in R Leonis

J. P. Fonfria, M. Santander-Garcia, J. Cernicharo et al
Astronomy and Astrophysics. Vol. 622
Journal article
2019

Discovery of two new magnesium-bearing species in IRC+10216: MgC3N and MgC4H

J. Cernicharo, C. Cabezas, J. R. Pardo et al
Astronomy and Astrophysics. Vol. 630
Journal article
2019

IRC+10 degrees 216 mass loss properties through the study of lambda 3 mm emission

Luis Velilla Prieto, J. Cernicharo, M. Agundez et al
Astronomy and Astrophysics. Vol. 629
Journal article
2019

Discovery of the first Ca-bearing molecule in space: CaNC

J. Cernicharo, Luis Velilla Prieto, M. Agundez et al
Astronomy and Astrophysics. Vol. 627
Journal article
2019

Hints of the Existence of C-rich Massive Evolved Stars

Guillermo Quintana-Lacaci, Jose Cernicharo, Marcelino Agundez et al
Astrophysical Journal. Vol. 876 (2)
Journal article
2018

Circumstellar chemistry of Si-C bearing molecules in the C-rich AGB star IRC+10216

Luis Velilla Prieto, Jose Cernicharo, M. Agundez et al
Proceedings of the International Astronomical Union. Vol. 14, p. 535-537
Paper in proceeding

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