Zobrazeno 1 - 10
of 601
pro vyhledávání: '"A. Gómez Garrido"'
Autor:
Taniguchi, Kotomi, Gorai, Prasanta, Tan, Jonathan C., Gomez-Garrido, Miguel, Fedriani, Ruben, Yang, Yao-Lun, Sridharan, T. K., Tanaka, Kei, Saito, Masao, Zhang, Yichen, Morgan, Lawrence, Cosentino, Giuliana, Law, Chi-Yan
Publikováno v:
A&A 692, A65 (2024)
Evidence for similar chemical characteristics around low- and high-mass protostars has been found: in particular, a variety of carbon-chain species and complex organic molecules (COMs) are formed around them. On the other hand, the chemical compositi
Externí odkaz:
http://arxiv.org/abs/2410.23392
Autor:
Gómez-Garrido, M., Bujarrabal, V., Alcolea, J., Castro-Carrizo, A., Mikołajewska, J., Santander-García, M.
Symbiotic systems often include an asymptotic giant branch (AGB) star and a hot compact companion, such as a white dwarf, that are in close interaction. Due to the intense ultraviolet emission from the hot companion, the molecular content of circumst
Externí odkaz:
http://arxiv.org/abs/2408.06033
Publikováno v:
Migraciones, Iss 61, Pp 1-25 (2024)
La distribución de los cuidados a la infancia procurados por personas que trascienden la familia nuclear es una práctica habitual entre las familias senegalesas y de otros países de África occidental. Estas formas de cuidado tienen un papel centr
Externí odkaz:
https://doaj.org/article/427ebfd2a1ef43a2b83553952ee14883
Publikováno v:
A&A 671, A80 (2023)
There is a class of binary post-asymptotic giant branch (post-AGB) stars that exhibit remarkable near-infrared (NIR) excess. These stars are surrounded by disks with Keplerian or quasi-Keplerian dynamics and outflows composed of gas escaping from the
Externí odkaz:
http://arxiv.org/abs/2301.06965
Autor:
Cava, I. Gallardo, Bujarrabal, V., Alcolea, J., Gómez-Garrido, M., Castro-Carrizo, A., Van Winckel, H., Santander-García, M.
Publikováno v:
Astronomy 2022, 1(2), 84-92
There is a class of binary post-AGB stars (binary system including a post-AGB star) that are surrounded by Keplerian disks and outflows resulting from gas escaping from the disk. To date, there are seven sources that have been studied in detail throu
Externí odkaz:
http://arxiv.org/abs/2208.02846
Autor:
Davalos-Yerovi, V., Gómez-Garrido, A., Garcia-Gutiérrez, R., Berastegui, C., Pujol-Blaya, V., Launois, P., Tejero-Sánchez, M., Canut, B., Curbelo, Y.G., Sánchez-Rodríguez, D.
Publikováno v:
In Rehabilitación October-December 2024 58(4)
Publikováno v:
A&A 659, A134 (2022)
Context. There is a class of binary post-asymptotic giant branch (post-AGB) stars that exhibit remarkable near-infrared (NIR) excess. Such stars are surrounded by Keplerian or quasi-Keplerian disks, as well as extended outflows composed of gas escapi
Externí odkaz:
http://arxiv.org/abs/2202.02106
Autor:
Martire Angélica Terrero Turbí, Melisa Gómez-Garrido, Oumaima El bied, José Gregorio Cuevas Bencosme, Ángel Faz Cano
Publikováno v:
Agriculture, Vol 14, Iss 10, p 1788 (2024)
Spain has been the largest pork producer in the EU in recent years, leading to significant pig slurry (PS) production that requires proper management to prevent environmental impacts. The objectives of this study were to quantify greenhouse gas (GHG)
Externí odkaz:
https://doaj.org/article/4cf8fc643c8c40468cee87192e2861df
Autor:
Pardo, J. R., Cernicharo, J., Tercero, B., Cabezas, C., Bermúdez, C., Agúndez, M., Gallego, J. D., Tercero, F., Gómez-Garrido, M., de Vicente, P., López-Pérez, J. A.
Context. IRC+10216, the carbon-rich envelope of the asymptotic giant branch (AGB) star CW Leo, is one of the richest molecular sources in the sky. Available spectral surveys below 51 GHz are more than 25 years old and new work is needed. Aims. Charac
Externí odkaz:
http://arxiv.org/abs/2111.02902
Autor:
Gómez-Garrido, A., Planas-Pascual, B., Launois, P., Pujol-Blaya, V., Dávalos-Yerovi, V., Berastegui-García, C., Esperidon-Navarro, C., Simon-Talero, C., Deu-Martin, M., Sacanell-Lacasa, J., Ciurana-Ayora, P., Ballesteros-Reviriego, G., Bello-Rodriguez, I., Roman-Broto, A.
Publikováno v:
In Rehabilitación July-September 2024 58(3)