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Akademický článek
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Akademický článek
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The main interest of the science team for the exploitation of the MEGARA instrument at the 10.4m Gran Telescopio Canarias (GTC) is devoted to the study of nearby galaxies. The focus lies on researching the history of star formation, and the chemical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1648::eae0b45048a3df213799f605f1ffaac7
https://hdl.handle.net/10481/81635
https://hdl.handle.net/10481/81635
Autor:
Anan Lu, Hope Boyce, Daryl Haggard, Martin Bureau, Fu-Heng Liang, Lijie Liu, Woorak Choi, Michele Cappellari, Laurent Chemin, Mélanie Chevance, Timothy A Davis, Laurent Drissen, Jacob S Elford, Jindra Gensior, J M Diederik Kruijssen, Thomas Martin, Etienne Massé, Carmelle Robert, Ilaria Ruffa, Laurie Rousseau-Nepton, Marc Sarzi, Gabriel Savard, Thomas G Williams
Publikováno v:
Lu, A, Boyce, H, Haggard, D, Bureau, M, Liang, F H, Liu, L, Choi, W, Cappellari, M, Chemin, L, Chevance, M, Davis, T A, Drissen, L, Elford, J S, Gensior, J, Diederik Kruijssen, J M, Martin, T, Masse, E, Robert, C, Ruffa, I, Rousseau-Nepton, L, Sarzi, M, Savard, G & Williams, T G 2022, ' WISDOM project-XI. Star formation efficiency in the bulge of the AGN-host Galaxy NGC 3169 with SITELLE and ALMA ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 4, pp. 5035-5055 . https://doi.org/10.1093/mnras/stac1583
The star formation efficiency (SFE) has been shown to vary across different environments, particularly within galactic starbursts and deep within the bulges of galaxies. Various quenching mechanisms may be responsible, ranging from galactic dynamics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf4f106343a224e921fb9d6efb2f495d
https://ora.ox.ac.uk/objects/uuid:f91736a9-c5d9-4412-a02c-435497bf0278
https://ora.ox.ac.uk/objects/uuid:f91736a9-c5d9-4412-a02c-435497bf0278
Autor:
Mauri J Valtonen, Lankeswar Dey, S Zola, S Ciprini, M Kidger, T Pursimo, A Gopakumar, K Matsumoto, K Sadakane, D B Caton, K Nilsson, S Komossa, M Bagaglia, A Baransky, P Boumis, D Boyd, A J Castro-Tirado, B Debski, M Drozdz, A Escartin Pérez, M Fiorucci, F Garcia, K Gazeas, S Ghosh, V Godunova, J L Gomez, R Gredel, D Grupe, J B Haislip, T Henning, G Hurst, J Janík, V V Kouprianov, H Lehto, A Liakos, S Mathur, M Mugrauer, R Naves Nogues, G Nucciarelli, W Ogloza, D K Ojha, U Pajdosz-Śmierciak, S Pascolini, G Poyner, D E Reichart, N Rizzi, F Roncella, D K Sahu, A Sillanpää, A Simon, M Siwak, F C Soldán Alfaro, E Sonbas, G Tosti, V Vasylenko, J R Webb, P Zielinski
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Full list of authors: Valtonen, Mauri J.; Dey, Lankeswar; Zola, S.; Ciprini, S.; Kidger, M.; Pursimo, T.; Gopakumar, A.; Matsumoto, K.; Sadakane, K.; Caton, D. B.; Nilsson, K.; Komossa, S.; Bagaglia, M.; Baransky, A.; Boumis, P.; Boyd, D.; Castro-Tir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f6b2e71c14159b2a0e832d0152922e2
http://hdl.handle.net/10261/278884
http://hdl.handle.net/10261/278884
Autor:
V. Kalinova, D. Colombo, S. F. Sánchez, E. Rosolowsky, K. Kodaira, R. García-Benito, S. E. Meidt, T. A. Davis, A. B. Romeo, S.-Y. Yu, R. González Delgado, E. A. D. Lacerda
Publikováno v:
ASTRONOMY & ASTROPHYSICS
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the orig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::00d3ccd527576f6f6b416fe26e35d944
http://arxiv.org/abs/2207.03872
http://arxiv.org/abs/2207.03872
Autor:
N. Cardiel, África Castillo-Morales, A. Gil de Paz, J. Gallego, A. Prez-Calpena, I. Martínez-Delgado, P. Gómez-Alvarez, Sergio Pascual, Jorge Iglesias-Páramo, M. L. García-Vargas, Bililign T. Dullo, Cristina Catalán-Torrecilla, R. Cedazo, M. Chamorro-Cazorla, Eleazar R. Carrasco
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense. Archivo Institucional de la UCM
Context. This paper aims to determine the capabilities of the MEGARA spectrograph at the Gran Telescopio Canarias (GTC), which is an optical integral-field unit, for studying stellar populations. We also aim to exploit its combination of high spectra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::992fb26586f2f08c899d2027924b0d79
http://hdl.handle.net/10261/267160
http://hdl.handle.net/10261/267160
Publikováno v:
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 649, pp.A42. ⟨10.1051/0004-6361/202040245⟩
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 649, pp.A42. ⟨10.1051/0004-6361/202040245⟩
Context. Brightest cluster galaxies (BCGs) grow by accreting numerous smaller galaxies, and can be used as tracers of cluster formation and evolution in the cosmic web. However, there is still controversy regarding the main epoch of formation of BCGs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2669531d795a32fda1918632925900e8
http://hdl.handle.net/10261/246897
http://hdl.handle.net/10261/246897
Publikováno v:
Digibug. Repositorio Institucional de la Universidad de Granada
Consorcio Madroño
Consorcio Madroño
JMA acknowledge support from the Spanish Ministerio de Economia y Competitividad (MINECO) by the grant AYA2017-83204-P and the Programa Operativo FEDER Andalucia 2014-2020 in collaboration with the Andalucian Office for Economy and Knowledge. AdLC ac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::050809ebf394c358b01b17b8256a1bbe
http://hdl.handle.net/10481/74167
http://hdl.handle.net/10481/74167
Autor:
Sara Cazzoli, Eduardo González-Alfonso, Fernando Rico-Villas, Matthew L. N. Ashby, C. Yang, K. P. Stewart, Luis Colina, Howard A. Smith, Jesús Martín-Pintado, Almudena Alonso-Herrero, Jacqueline Fischer, Miguel Pereira-Santaella, Santiago García-Burillo
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)
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Galaxies with nuclear bars are believed to efficiently drive gas inward, generating a nuclear starburst and possibly an active galactic nucleus. We confirm this scenario for the isolated, double-barred, luminous infrared galaxy ESO 320-G030 based on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4d49a2aca5bfefec37c1e6f2ba0be36b
http://hdl.handle.net/10261/239125
http://hdl.handle.net/10261/239125