Table 1.
Basic properties of FCC 47 and its NSC.
| FCC 47 | Notes | |
|---|---|---|
| Morphological type | S0 | 1 |
| Distance [Mpc] | 18.3 ± 0.6 | 2 |
| Physical scale [pc arcsec−1] | 88.72 | |
| Inclination [°] | 47 ± 4 | 3 |
| Effective radius [kpc] | 2.40 | 4 |
| Galaxy stellar mass [M⊙] | (1.0 ± 0.1) ×1010 | 5 |
| σcen [km s−1] | 106 ± 5 | 6 |
| NSC | Notes | |
| Effective radius [pc] | 66.5 ± 11.1 | |
| Effective radius [″] | 0.75 ± 0.125 | 7 |
| NSC mass [M⊙] | 7.3 ± 1.2 × 108 | 8 |
Notes. (1) de Vaucouleurs et al. (1991). (2) Blakeslee et al. (2009). (3) Thater et al. (2023). (4) derived by applying the mge_half_light_radius routine of the JamPy package on the MGE of the stellar mass model (Section 2.1) (Cappellari 2002, 2008. (5) Thater et al. (2023) using a dynamical Schwarzschild orbit-superposition model with varying stellar populations and varying IMF. (6) Thater et al. (2023); (7) Turner et al. (2012), measured in the F475W Filter (≈g−band); (8) Fahrion et al. (2019) photometric mass using stellar population models.
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.