Table 1
Properties of the CALIFA prolate rotators.
| Name | T/G | d | M∗ | re | Ψ |
| (Mpc) | (1011M⊙) | (kpc) | (deg) | ||
|
|
|||||
| LSBCF560-04 | E5/BCG | 238 | 7.1 ± 0.6a | 17.9 | 57 ± 5 |
| NGC 0647 | E7/in a group | 184 | 3.7 ± 0.3a | 8.7 | 72 ± 3 |
| NGC 0810 | E5/in a pair | 110 | 2.12 b |
9.3 | 87 ± 2 |
| NGC 2484 | E4/BCG | 192 | 5.0 ± 0.5 a | 12.5 | 52 ± 4 |
| NGC 4874 | E0/BCG | 102 | 2.8 b |
12.4 | 86 ± 5 |
| NGC 5216 | E0/in a pair | 42 | 0.230 b |
4.1 | 66 ± 5 |
| NGC 5485 | E5/in a group | 27 | 0.9 b |
4.1 | 80 ± 3 |
| NGC 6173 | E6/BCG | 126 | 2.5 b |
30.5 | 80 ± 2 |
| NGC 6338 | E5/BCG | 117 | 3.0 b |
17.0 | 36 ± 4 |
| UGC 10695* | E5/in a group | 120 | 2.7 ± 0.2a | 15.7 | 87 ± 2 |
Notes. Column 1: name. Column 2: Hubble type T, as in Walcher et al. (2014), and group membership G (NED/SIMBAD). Column 3: redshift-based distance in Mpc. Column 4: available stellar mass estimates, and Column 5: effective radius, determined by growth-curve analysis of SDSS images of each galaxy, as in Walcher et al. (2014). Column 6: global kinematic misalignment angle Ψ. Cosmological angular size distances are calculated by adopting H0 = 70 km s-1 Mpc-1, Ωm = 0.3, ΩΛ = 0.7.
from WISE photometry by Norris et al. (2016),
from CALIFA DR3, as in Walcher et al. (2014).
UGC 10695 is listed as a further candidate, showing evidence for prolate rotation.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.