The empty ring galaxy ESO 474-G040
Author(s) -
N. Brosch,
P. Väisänen,
A. Y. Kniazev,
А. В. Моисеев
Publication year - 2015
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stv1245
Subject(s) - physics , galaxy , ring (chemistry) , astrophysics , metallicity , stellar population , telescope , stars , astronomy , spectroscopy , very large telescope , population , line (geometry) , kinematics , star formation , geometry , classical mechanics , chemistry , demography , organic chemistry , mathematics , sociology
We describe observations of the apparently empty ring galaxy ESO 474-G040 obtained with the Southern African Large Telescope (SALT). The observations, consisting of imaging, long-slit spectroscopy and Fabry-Perot mapping of the H-alpha line, allow determining the ring kinematics as well as estimating the metallicity of the ring and the stellar population composition in its various parts. We propose that the object could best be understood as being the result of a past merger of disk galaxies, which formed a gas ring that subsequently disrupted via the bead instability and is presently forming stars.
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