R
R. Cid Fernandes
Researcher at Universidade Federal de Santa Catarina
Publications - 159
Citations - 11466
R. Cid Fernandes is an academic researcher from Universidade Federal de Santa Catarina. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 55, co-authored 154 publications receiving 10512 citations. Previous affiliations of R. Cid Fernandes include Spanish National Research Council & Johns Hopkins University.
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Journal ArticleDOI
Multiwavelength study of the nuclei of a volume-limited sample of galaxies – II. Optical, infrared and radio observations
TL;DR: In this article, the authors presented optical and infrared broad-band images, radio maps, and optical spectroscopy for the nuclear region of a sample of nearby galaxies, which were drawn from a complete volume-limited sample for which they have already presented X-ray imaging.
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The CALIFA view on stellar angular momentum across the Hubble sequence
Jesús Falcón-Barroso,Jesús Falcón-Barroso,G. van de Ven,Mariya Lyubenova,Jairo Méndez-Abreu,Jairo Méndez-Abreu,J. A. L. Aguerri,J. A. L. Aguerri,Begoña García-Lorenzo,Begoña García-Lorenzo,S. Bekeraite,Sebastián F. Sánchez,Bernd Husemann,R. García-Benito,R. M. González Delgado,D. Mast,C. J. Walcher,Stefano Zibetti,Ling Zhu,Jorge K. Barrera-Ballesteros,Lluís Galbany,Patricia Sanchez-Blazquez,R. Singh,R. C. E. van den Bosch,Vivienne Wild,Joss Bland-Hawthorn,R. Cid Fernandes,A. de Lorenzo-Cáceres,A. de Lorenzo-Cáceres,Anna Gallazzi,R. A. Marino,I. Márquez,Reynier Peletier,Enrique Pérez,I. Pérez,Martin Roth,F. F. Rosales-Ortega,Tomás Ruiz-Lara,Tomás Ruiz-Lara,Lutz Wisotzki,Bodo L. Ziegler +40 more
TL;DR: In this paper, the apparent stellar angular momentum of 300 galaxies across the Hubble sequence, using integral-field spectroscopic data from the CALIFA survey, was measured in different apertures.
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Spatially resolved mass-to-light from the CALIFA survey: Mass-to-light ratio vs. color relations
R. García-Benito,R. M. González Delgado,Enrique Pérez,R. Cid Fernandes,Samuel Sanchez,A. L. de Amorim +5 more
TL;DR: Support from the Spanish Ministerio de Economia y Competitividad, through projects AYA2016-77846-P, AYA2014-57490-P and AYA2010-15081, and Junta de Andalucia P12-FQM-2828, was provided by CONACYT (Mexico) grant CB-285080, and funding from the PAPIIT-DGAPA-IA101217 (UNAM) as mentioned in this paper.
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The many faces of LINER-like galaxies: a WISE view
TL;DR: In this article, the authors used the SDSS and WISE surveys to investigate the real nature of galaxies defined as LINERs in the BPT diagram, and found that a large fraction of LINER-like galaxies are emission-line retired galaxies, i.e. galaxies which have stopped forming stars and are powered by hot low-mass evolved stars (HOLMES).
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Unresolved Wind-Driven Shells and the Supersonic Velocity Dispersion in Giant HII Regions
TL;DR: In this paper, the authors evaluate the impact that winds may have on the structure of giant nebulae and on their supersonic velocity dispersion, and they show that a combination of a large number of unresolved wind-driven shells caused by massive stars could produce the integrated broad Gaussian profiles typical of giant HII regions.