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

Bibcode
2017IAUS..321..278R
DOI
10.1017/S1743921316009406
Ruiz-Lara, T.; Pérez, Isabel; Florido, Estrella; Sánchez-Blázquez, Patricia; Méndez-Abreu, Jairo; Lyubenova, Mariya; Falcón-Barroso, J.; Sánchez-Menguiano, Laura; Sánchez, Sebastián F.; CALIFA Team
Referencia bibliográfica

Formation and Evolution of Galaxy Outskirts, Proceedings of the International Astronomical Union, IAU Symposium, Volume 321, pp. 278-278

Advertised on:
3
2017
Número de autores
10
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro

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