Resolving double-peaked emission line galaxies using MaNGA: I. Mechanisms of star formation quenching

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作者：
Mazzilli Ciraulo, Barbara [1 ,2 ,3 ]
Melchior, Anne-Laure [1 ]
Combes, Françoise [1 ,4 ]
Maschmann, Daniel [1 ,5 ]
机构：
[1] Observatoire de Paris, PSL University, CNRS, Sorbonne Université, LERMA, Paris,75014, France
[2] Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn,VIC,3122, Australia
[3] ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
[4] Collège de France, 11 Place Marcelin Berthelot, Paris,75005, France
[5] Space Telescope Science Institute, 3700 San Martin Drive, Baltimore,MD,21218, United States
来源：
Astronomy and Astrophysics | 1600年 / 690卷
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