Zobrazeno 1 - 10
of 81
pro vyhledávání: '"M. Gómez-Garrido"'
Akademický článek
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Akademický článek
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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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::966f9141e0df8c02f74f20fcea6d70e9
http://arxiv.org/abs/2301.06965
http://arxiv.org/abs/2301.06965
Akademický článek
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Context. There is a class of binary post-asymptotic giant branch (post-AGB) stars that exhibit remarkable near-infrared excess. Such stars are surrounded by Keplerian or quasi-Keplerian disks, as well as extended outflows composed of gas escaping fro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b0b3fe496fd090ea1a22eccbc426c34
http://arxiv.org/abs/2202.02106
http://arxiv.org/abs/2202.02106
Autor:
Z. R. Weaver, Svetlana G. Jorstad, J. González García, B. Boccardi, Thomas P. Krichbaum, Michael Lindqvist, Jeffrey A. Hodgson, J. A. Zensus, M. Gómez Garrido, Jia-Hui Yang, S. Sanchez, Carolina Casadio, J. Y. Kim, Juha Kallunki, Alan P. Marscher, Nicholas R. MacDonald, Efthalia Traianou
Publikováno v:
Astronomy & Astrophysics
Controversial studies on the jet collimation profile of BL Lacertae (BL Lac), the eponymous blazar of BL Lac objects class, complicate the scenario in this already puzzling class of objects. Understanding the jet geometry, in connection with the jet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52b0bb36bb3c245916c6505110ef21a7
Autor:
M. Santander-García, A. Castro-Carrizo, Hyosun Kim, M. Gómez-Garrido, Valentin Bujarrabal, Marcelino Agúndez, J. Alcolea, Joanna Mikolajewska
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
17 pags., 16 figs.
Aims. We investigate the structure, dynamics, and chemistry of the molecule-rich nebula around the stellar symbiotic system R Aqr, which is significantly affected by the presence of a white dwarf (WD) companion. We study the e
Aims. We investigate the structure, dynamics, and chemistry of the molecule-rich nebula around the stellar symbiotic system R Aqr, which is significantly affected by the presence of a white dwarf (WD) companion. We study the e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::60ec6d04990149e8ad54acadcbb3dc48
Yebes 40 m radio telescope and the broad band NANOCOSMOS receivers at 7 mm and 3 mm for line surveys
Autor:
J. M. Serna, P. García-Carreño, Oscar García, J. A. López-Fernández, F. Tercero, Juan R. Pardo, Ricardo Amils, José Cernicharo, M. Santander-García, G. Gómez-Molina, B. Vaquero, Juan Daniel Gallego, Valentin Bujarrabal, J. M. Hernandez, F. Beltrán, J. González-García, J. A. López-Pérez, M. Gómez-Garrido, I. Malo, P. de Vicente, L. Barbas, C. Albo, I. Lopez-Fernandez, M. C. Diez, M. Patino-Esteban, Belén Tercero
Publikováno v:
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astron Astrophys
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astron Astrophys
22 pags., 27 figs., 6 tabs.
Context. Yebes 40 m radio telescope is the main and largest observing instrument at Yebes Observatory and is devoted to very long baseline interferometry (VLBI) and single-dish observations since 2010. It has been cov
Context. Yebes 40 m radio telescope is the main and largest observing instrument at Yebes Observatory and is devoted to very long baseline interferometry (VLBI) and single-dish observations since 2010. It has been cov
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c356a0b9bf01cfa53eaf628edf9ad14
http://arxiv.org/abs/2010.16224
http://arxiv.org/abs/2010.16224
Autor:
M. Gómez-Garrido, J. Alcolea, P. de Vicente, R. Soria-Ruiz, Valentin Bujarrabal, J. F. Desmurs
Context.Stars on the asymptotic giant branch (AGB) are long-period variables that present strong flux variations at almost all wavelengths, including the SiO maser lines. The periods of these variations are of 300–500 days in Mira-type stars and so
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd589b6fd7d632d8585802687bd2e5ca
http://arxiv.org/abs/2009.09771
http://arxiv.org/abs/2009.09771
Autor:
E. Delgado Mena, Paula Jofre, Andreas J. Korn, Gerard Gilmore, Rosaria Bonito, Lorenzo Monaco, Giovanni Carraro, Clare Worley, Sofia Randich, Ulrike Heiter, Sofia Feltzing, Simone Zaggia, D. Montes, Hugo M. Tabernero, F. Jiménez Esteban, Thomas Bensby, A. Hourihane, S. G. Sousa, Rodolfo Smiljanic, L. Prisinzano, L. Morbidelli, Antonio Frasca, V. Roccatagliata, Emilio J. Alfaro, A. Klutsch, M. L. Gutiérrez Albarrán, M. Gómez Garrido, A. C. Lanzafame, Emilio Marfil, Amelia Bayo, M. Van der Swaelmen, E. Franciosini, J. I. González Hernández, Anais Gonneau, Thomas Masseron, M. Baratella
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
E-Prints Complutense. Archivo Institucional de la UCM
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
E-Prints Complutense. Archivo Institucional de la UCM
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Full list of authors: Gutiérrez Albarrán, M. L.; Montes, D.; Gómez Garrido, M.; Tabernero, H. M.; González Hernández, J. I.; Marfil, E.; Frasca, A.; Lanzafame, A. C.; Klutsch, A.; Franciosini, E.; Randich, S.; Smiljanic, R.; Korn, A. J.; Gilmore
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34d9056ff4ebc0c2ed211a33edc93a32
http://hdl.handle.net/10261/228372
http://hdl.handle.net/10261/228372