Por favor, use este identificador para citar o enlazar a este item:
http://hdl.handle.net/10261/209172
COMPARTIR / EXPORTAR:
SHARE CORE BASE | |
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE | |
Título: | Morpho-kinematic properties of field S0 bulges in the CALIFA survey |
Autor: | Méndez-Abreu, J.; Aguerri, J.A.L.; Falcón-Barroso, Jesús; Ruiz-Lara, T.; Sánchez Menguiano, Laura; de Lorenzo-Cáceres, A.; Costantin, L.; Catalán-Torrecilla, C.; Zhu, L.; Sánchez-Blazquez, P.; Florido, E.; Corsini, E.M.; Wild, V.; Lyubenova, M.; van de Ven, G.; Sánchez, S. F.; Bland-Hawthorn, J.; Galbany, Lluís CSIC ORCID ; García-Benito, Rubén CSIC ORCID ; García-Lorenzo, B.; González Delgado, Rosa M. CSIC ORCID ; López-Sánchez, A.R.; Marino, R.A.; Márquez, Isabel CSIC ORCID; Ziegler, B. | Palabras clave: | Galaxies: bulges Galaxies: evolution Galaxies: formation Galaxies: kinematics and dynamics Galaxies: photometry Galaxies: structure |
Fecha de publicación: | 2018 | Editor: | Oxford University Press | Citación: | Monthly Notices of the Royal Astronomical Society 474: 1307-1334 (2018) | Resumen: | We study a sample of 28 S0 galaxies extracted from the integral field spectroscopic (IFS) survey Calar Alto Legacy Integral Field Area. We combine an accurate two-dimensional (2D) multicomponent photometric decomposition with the IFS kinematic properties of their bulges to understand their formation scenario. Our final sample is representative of S0s with high stellar masses (M*/M > 10). They lay mainly on the red sequence and live in relatively isolated environments similar to that of the field and loose groups. We use our 2D photometric decomposition to define the size and photometric properties of the bulges, as well as their location within the galaxies. We perform mock spectroscopic simulations mimicking our observed galaxies to quantify the impact of the underlying disc on our bulge kinematic measurements (λ and υ/σ).We compare our bulge corrected kinematic measurements with the results from Schwarzschild dynamical modelling. The good agreement confirms the robustness of our results and allows us to use bulge deprojected values of λ and υ/σ. We find that the photometric (n and B/T) and kinematic (υ/σ and λ) properties of our field S0 bulges are not correlated. We demonstrate that this morpho-kinematic decoupling is intrinsic to the bulges and it is not due to projection effects. We conclude that photometric diagnostics to separate different types of bulges (disc-like versus classical) might not be useful for S0 galaxies. The morpho-kinematics properties of S0 bulges derived in this paper suggest that they are mainly formed by dissipational processes happening at high redshift, but dedicated high-resolution simulations are necessary to better identify their origin.© 2017 The Author(s).Published by Oxford University Press on behalf of the Royal Astronomical Society | Versión del editor: | http://dx.doi.org/10.1093/mnras/stx2804 | URI: | http://hdl.handle.net/10261/209172 | DOI: | 10.1093/mnras/stx2804 | Identificadores: | doi: 10.1093/mnras/stx2804 issn: 1365-2966 |
Aparece en las colecciones: | (IAA) Artículos |
Ficheros en este ítem:
Fichero | Descripción | Tamaño | Formato | |
---|---|---|---|---|
IAA_2018stx2804.pdf | 4,61 MB | Adobe PDF | Visualizar/Abrir |
CORE Recommender
SCOPUSTM
Citations
32
checked on 18-abr-2024
WEB OF SCIENCETM
Citations
31
checked on 25-feb-2024
Page view(s)
189
checked on 12-may-2024
Download(s)
141
checked on 12-may-2024
Google ScholarTM
Check
Altmetric
Altmetric
NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.