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No direct coupling between bending of galaxy disc stellar age and light profiles as seen from CALIFA

Published online by Cambridge University Press:  21 March 2017

Tomás Ruiz-Lara ,
Isabel Pérez ,
Estrella Florido ,
Patricia Sánchez-Blázquez ,
Jairo Méndez-Abreu ,
Mariya Lyubenova ,
Jesús Falcón-Barroso ,
Laura Sánchez-Menguiano ,
Sebastián F. Sánchez  and
the CALIFA team
Tomás Ruiz-Lara
Affiliation:
Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada, Spain. email: [email protected], [email protected], [email protected] Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, E-18071
Isabel Pérez
Affiliation:
Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada, Spain. email: [email protected], [email protected], [email protected] Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, E-18071
Estrella Florido
Affiliation:
Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada, Spain. email: [email protected], [email protected], [email protected] Instituto Carlos I de Física Teórica y computacional, Universidad de Granada, E-18071
Patricia Sánchez-Blázquez
Affiliation:
Dpto. de Física Teórica, Universidad Autónoma de Madrid, E-28049 Cantoblanco, Spain
Jairo Méndez-Abreu
Affiliation:
School of Physics and Astronomy, University of St Andrews, St Andrews, UK
Mariya Lyubenova
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, Groningen, the Netherlands
Jesús Falcón-Barroso
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
Laura Sánchez-Menguiano
Affiliation:
Dpto. de Física Teórica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, E-18071 Granada, Spain. email: [email protected], [email protected], [email protected] Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain
Sebastián F. Sánchez
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, México D.F., Mexico
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Recent theoretical and observational works claim the existence of galaxies with a characteristic age profile consisting on a negative radial trend followed by a smooth age upturn in its outskirts (“U-shape”). This shape has been generally related to down-bending light distributions; however, the existence of a real link between observed Surface Brightness (SB) profiles and changes in stellar properties such as age is still unclear.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S321: Formation and Evolution of Galaxy Outskirts , March 2016 , pp. 278
Copyright
Copyright © International Astronomical Union 2017 

References

Sánchez, S. F., et al. 2012, A&A, 538, A8 Google Scholar
Ruiz-Lara, T., Pérez, I., Florido, E., Sánchez-Blázquez, P., et al. 2016, MNRAS, 456L, 35 Google Scholar