Univ.-Prof. Dr. Bodo Ziegler Leiter des Instituts Seminar über “Galaxy structure as a tracer of accretion and interaction history” The morphology of galaxies is closely related to both their star-formation anddynamical histories. I will describe a collection of studies which use novel measurements of internal structure to infer the long- and short-timescale evolutionary processes affecting different types of galaxies. These measurements include spiral arm properties derived from Galaxy Zoo visual inspection of SDSS images, and MegaMorph multi-wavelength profile fits to both survey imaging and integral-field spectroscopic data. I will discuss the role of interactions and star-formation in determining spiral structure, present clear signatures of the contrasting inside-out formation of disks and spheroids, and highlight the outside-in nature of galaxy quenching. Von Dr. Steven Bamford University of Nottingham, Nottingham Montag, 21. November 2016, um 15:00 Uhr im HS des Institutes für Astrophysik, Türkenschanzstraße 17, 1180 Wien Institut für Astrophysik — Türkenschanzstraße 17 — A-1180 Wien, AUSTRIA Tel.: +43 (1) 4277 - 53825 — GSM: +43 (664) 60277 - 53825 — Fax: +43 (1) 4277 - 9518 E-mail: [email protected] — URL: http://homepage.univie.ac.at/bodo.ziegler /
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