Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 477, Issue 4, Pages 4711-4737Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/sty504
Keywords
galaxies: elliptical and lenticular, cD; galaxies: evolution; galaxies: formation; galaxies: kinematics and dynamics; galaxies: spiral
Categories
Funding
- UK Science and Technology Facilities Council [ST/N504233/1]
- Royal Society University Research Fellowship
- Leverhulme Trust Early Career Fellowship
- Alfred P. Sloan Foundation
- U.S. Department of Energy Office of Science
- Center for High-Performance Computing at the University of Utah
- Carnegie Institution for Science
- Carnegie Mellon University
- Chilean Participation Group
- French Participation Group
- Harvard-Smithsonian Center for Astrophysics
- Instituto de Astrofisica de Canarias
- Johns Hopkins University
- Kavli Institute for the Physics and Mathematics of the Universe (IPMU) / University of Tokyo
- Lawrence Berkeley National Laboratory
- Leibniz Institut fr Astrophysik Potsdam (AIP)
- Max-Planck-Institut fr Astronomie (MPIA Heidelberg)
- Max-Planck-Institut fr Astrophysik (MPA Garching)
- Max-Planck-Institut fr Extraterrestrische Physik (MPE)
- National Astronomical Observatories of China
- New Mexico State University
- New York University
- University of Notre Dame
- Observatrio Nacional /MCTI
- Ohio State University
- Pennsylvania State University
- Shanghai Astronomical Observatory
- United Kingdom Participation Group
- Universidad Nacional Autnoma de Mexico
- University of Arizona
- University of Colorado Boulder
- University of Oxford
- University of Portsmouth
- University of Utah
- University of Virginia
- University of Washington
- University of Wisconsin
- Vanderbilt University
- Yale University
- National Aeronautics and Space Administration
- National Science Foundation
- STFC [ST/P000649/1, ST/N504233/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/P000649/1, 1659482] Funding Source: researchfish
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We measure lambda R-e, a proxy for galaxy specific stellar angular momentum within one effective radius, and the ellipticity, is an element of, for about 2300 galaxies of all morphological types observed with integral field spectroscopy as part of the Mapping Nearby Galaxies at Apache Point Observatory survey, the largest such sample to date. We use the (lambda R-e, is an element of) diagram to separate early-type galaxies into fast and slow rotators. We also visually classify each galaxy according to its optical morphology and two-dimensional stellar velocity field. Comparing these classifications to quantitative lambda R-e measurements reveals tight relationships between angular momentum and galaxy structure. In order to account for atmospheric seeing, we use realistic models of galaxy kinematics to derive a general approximate analytic correction for lambda R-e. Thanks to the size of the sample and the large number of massive galaxies, we unambiguously detect a clear bimodality in the ( lambda R-e, is an element of) diagram which may result from fundamental differences in galaxy assembly history. There is a sharp secondary density peak inside the region of the diagram with low lambda R-e is an element of < 0.4, previously suggested as the definition for slow rotators. Most of these galaxies are visually classified as non-regular rotators and have high velocity dispersion. The intrinsic bimodality must be stronger, as it tends to be smoothed by noise and inclination. The large sample of slow rotators allows us for the first time to unveil a secondary peak at +/- 90 degrees in their distribution of the misalignments between the photometric and kinematic position angles. We confirm that genuine slow rotators start appearing above M >= 2 x 10(11)M(circle dot) where a significant number of high-mass fast rotators also exist.
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