Investigating the Formation and Evolution of Massive Disc Galaxies with the MUSE TIMER Project

Bibcode
2018Msngr.173...28G
DOI
10.18727/0722-6691/5095
Gadotti, D. A.; Sánchez-Blázquez, P.; Falcón-Barroso, J.; Husemann, B.; Seidel, M.; Leaman, R.; Leung, G.; van de Ven, G.; Querejeta, M.; Fragkoudi, F.; de Lorenzo-Cáceres, A. d.; Méndez-Abreu, J.; Pérez, I.; Kim, T.; Martinez-Valpuesta, I.; Coelho, P.; Donohoe-Keyes, C.; Martig, M.; Neumann, J.
Bibliographical reference

The Messenger, vol. 173, p. 28-32

Advertised on:
9
2018
Number of authors
19
IAC number of authors
4
Citations
1
Refereed citations
1
Description
The Time Inference with MUSE in Extragalactic Rings (TIMER) project is a survey using the integral-field spectrograph Multi Unit Spectroscopic Explorer (MUSE) on the VLT to study 24 nearby barred galaxies with prominent central structures, such as nuclear rings or inner discs. One of our main goals is to estimate the cosmic epoch when galaxy discs settle, leading to the formation of bars. This is also the onset of a phase in the history of the Universe during which secular evolution processes in galaxies become important. We illustrate the quality of the data with some first results and describe the legacy potential of the survey.
Type
Non-refereed

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