期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 483, 期 2, 页码 2413-2423出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/sty3268
关键词
galaxies: evolution; galaxies: stellar content; galaxies: structure
资金
- Southern African Large Telescope (SALT) [2014-2-MLT-001, 2015-2-MLT-002]
- National Research Foundation (NRF) of South Africa
- Russian Science Foundation [17-72-20119]
- Russian Foundation for Basic Research [16-02-00649]
- M.V. Lomonosov Moscow State University Program of Development
Galactic stellar discs, such as that of the Milky Way, have usually a complex structure consisting of a thin and a thick component. The study of galactic disc sub-structures and their differences can shed light on the galaxy assembling processes and their evolution. However, due to observational difficulties there is a lack of information about the stellar populations of the thick disc components in external galaxies. Here, we investigate three edge-on early-type disc galaxies in the Fornax cluster (IC 335, NGC1380A, NGC1381) by using publicly available photometrical data and our newdeep long-slit spectroscopy along galactic mid-planes obtained with the 10-m SALT telescope. We report that significant changes of the stellar population properties beyond the radius where photometrical profiles demonstrate a knee are caused by an increasing thick disc contribution. Stellar population properties in the outermost thick-disc dominated regions demonstrate remarkably old ages and a low metallicity. We interpret these findings as a consequence of star formation quenching in the outermost regions of the discs due to ram pressure gas stripping from the disc periphery at the beginning of the cluster assembly while subsequent star formation occurring in the inner discs being gradually extinguished by starvation.
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