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![]() |
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![]() |
12.4 | 86 ± 5 |
NGC 5216 | E0/in a pair | 42 | 0.230![]() |
4.1 | 66 ± 5 |
NGC 5485 | E5/in a group | 27 | 0.9![]() |
4.1 | 80 ± 3 |
NGC 6173 | E6/BCG | 126 | 2.5![]() |
30.5 | 80 ± 2 |
NGC 6338 | E5/BCG | 117 | 3.0![]() |
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.
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