Zobrazeno 1 - 10
of 100
pro vyhledávání: '"L. Velilla-Prieto"'
Autor:
L. Velilla-Prieto, J. P. Fonfría, M. Agúndez, A. Castro-Carrizo, M. Guélin, G. Quintana-Lacaci, I. Cherchneff, C. Joblin, M. C. McCarthy, J. A. Martín-Gago, J. Cernicharo
Publikováno v:
Nature. 617:696-700
Akademický článek
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Autor:
C. Sanchez Contreras, J. Alcolea, R. Rodriguez Cardoso, V. Bujarrabal, A. Castro-Carrizo, G. Quintana-Lacaci, L. Velilla-Prieto, M. Santander-Garcia
29 pags., 18 figs., 3 tabs. 1 app.
We present a set of Atacama Large Millimeter/submillimeter Array (ALMA) continuum and molecular line emission maps at ~1 mm wavelengths of OH 231.8+4.2. This is a well studied bipolar nebula around an asymptoti
We present a set of Atacama Large Millimeter/submillimeter Array (ALMA) continuum and molecular line emission maps at ~1 mm wavelengths of OH 231.8+4.2. This is a well studied bipolar nebula around an asymptoti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e98a95a351939c185f6c25d7e6fe1ae7
http://hdl.handle.net/10261/305214
http://hdl.handle.net/10261/305214
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
C. Sánchez Contreras, J. Alcolea, R. Rodríguez-Cardoso, V. Bujarrabal, A. Castro-Carrizo, L. Velilla-Prieto, G. Quintana-Lacaci, M. Santander-García, M. Agúndez, J. Cernicharo
Publikováno v:
Proceedings of the International Astronomical Union. 16:301-307
We present interferometric continuum and molecular line emission maps obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) of OH231.8+4.2, a well studied bipolar nebula around an asymptotic giant branch (AGB) star that is key to unde
The nucleosynthesis production of fluorine (F) is still a matter of debate. Asymptotic giant branch (AGB) stars are one of the main candidates for F production. However, their contribution to the total F budget is not fully known due to the lack of o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f86cc843fe298b9b08de66c5b4640b79
http://hdl.handle.net/10852/95014
http://hdl.handle.net/10852/95014
Autor:
G. Quintana-Lacaci, L. Velilla-Prieto, M. Agúndez, J. P. Fonfría, J. Cernicharo, L. Decin, A. Castro-Carrizo
12 pags., 10 figs. 2 tabs.
Red supergiant stars (RSGs, Minit = 10-40Msun) are known to eject large amounts of material, as much as half of their initial mass during this evolutionary phase. However, the processes powering the mass ejection in lo
Red supergiant stars (RSGs, Minit = 10-40Msun) are known to eject large amounts of material, as much as half of their initial mass during this evolutionary phase. However, the processes powering the mass ejection in lo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e4395c399008da440b3f4475ad9301b
Publikováno v:
Astron Astrophys
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
22 pags., 3 figs., 5 tabs.
Aims. We aim to determine the abundances of SiO, CS, SiS, SO, and SO2 in a large sample of oxygen-rich asymptotic giant branch (AGB) envelopes covering a wide range of mass loss rates to investigate the potential role
Aims. We aim to determine the abundances of SiO, CS, SiS, SO, and SO2 in a large sample of oxygen-rich asymptotic giant branch (AGB) envelopes covering a wide range of mass loss rates to investigate the potential role
Autor:
L. Velilla-Prieto, Carlos Cabezas, Celina Bermúdez, M. Guelin, G. Quintana-Lacaci, Belén Tercero, Marcelino Agúndez, J. D. Gallego, José Cernicharo, José Pablo Fonfría, Juan R. Pardo
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astron Astrophys
instname
Astron Astrophys
12 pags., 8 figs., 8 tabs.-- Section: Letters to the Editor
Observations of IRC +10216 with the Yebes 40 m telescope between 31 and 50 GHz have revealed more than 150 unidentified lines. Some of them can be grouped into a new series of 26 double
Observations of IRC +10216 with the Yebes 40 m telescope between 31 and 50 GHz have revealed more than 150 unidentified lines. Some of them can be grouped into a new series of 26 double
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2532815ef44f2f0956bbc52b2d6773c
http://hdl.handle.net/10261/222403
http://hdl.handle.net/10261/222403
Autor:
J, Cernicharo, C, Cabezas, J R, Pardo, M, Agúndez, C, Bermúdez, L, Velilla-Prieto, F, Tercero, J A, López-Pérez, J D, Gallego, J P, Fonfría, G, Quintana-Lacaci, M, Guélin, Y, Endo
Publikováno v:
Astronomy and astrophysics. 630
We report on the detection of two series of harmonically related doublets in IRC +10216. From the observed frequencies, the rotational constant of the first series is B = 1380.888 MHz and that of the second series is B = 1381.512 MHz. The two series