Table B.1
Sample of starbursting dwarfs: structural and dynamical properties.
| Name | Dist | Method | Ref. | M R |
|
Rd | Ref. | i | VRd | Vlast | Rlast | Ref. | VRd/Rd |
| (Mpc) | (mag) | (mag/′′2) | (kpc) | (°) | (km s-1) | (km s-1) | (kpc) | (km s-1/kpc) | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
|
|
|||||||||||||
| NGC 1705α | 5.1 ± 0.6 | TRGB | a | −16.3 ± 0.2 | 21.1 ± 0.1 | 0.46 | i | 45 ± 5 | 58 ± 8 | 71 ± 10 | 5.7 | i | 126 ± 25 |
| NGC 2366 | 3.2 ± 0.4 | Ceph | b | −16.6 ± 0.3 | 22.5 ± 0.2 | 1.36 | j | 68 ± 5 | 30 ± 2 | 49 ± 6 | 5.9 | i | 22 ± 3 |
| NGC 2915β | 3.8 ± 0.4 | TRGB | c | −15.9 ± 0.2 | 20.5 ± 0.1 | 0.46 | k | 52 ± 3 | 32 ± 15 | 85 ± 5 | 9.3 | m | 70 ± 33 |
| NGC 4068 | 4.3 ± 0.1 | TRGB | d | −15.7 ± 0.1 | 21.8 ± 0.1 | 0.56 | j | 44 ± 6 | 13 ± 4 | 39 ± 5 | 2.3 | i | 23 ± 8 |
| NGC 4214α | 2.7 ± 0.2 | TRGB | d | −17.8 ± 0.2 | 20.3 ± 0.1 | 0.70 | j | 30 ± 10 | 64 ± 8 | 81 ± 9 | 4.8 | i | 91 ± 31 |
| NGC 6789 | 3.6 ± 0.2 | TRGB | e | −15.1 ± 0.1 | 21.1 ± 0.2 | 0.23 | i | 43 ± 7 | 23 ± 4 | 57 ± 9 | 0.7 | i | 100 ± 22 |
| UGC 4483 | 3.2 ± 0.2 | TRGB | f | −13.0 ± 0.1 | 22.7 ± 0.1 | 0.20 | i | 58 ± 3 | 10 ± 3 | 19 ± 2 | 1.2 | n | 50 ± 15 |
| I Zw 18γ | 18.2 ± 1.4 | TRGB | g | −15.0 ± 0.2 | 20.5 ± 0.2 | 0.15 | l | 70 ± 4 | 25 ± 10 | 38 ± 4 | 0.8 | o | 167 ± 60 |
| I Zw 36 | 5.9 ± 0.5 | TRGB | h | −14.9 ± 0.1 | 22.5 ± 0.2 | 0.29 | i | 67 ± 3 | 16 ± 2 | 29 ± 2 | 1.1 | i | 55 ± 8 |
Notes.
We adopted the rotation curve derived by Elson et al. (2010) assuming a constant inclination of 52°.
The optical parameters have been derived by Papaderos et al. (2002) after subtracting the Hα emission.
Reference. (a) Tosi et al. (2001); (b) Tolstoy et al. (1995); (c) Karachentsev et al. (2003); (d) Jacobs et al. (2009); (e) Drozdovsky et al. (2001); (f) Izotov & Thuan (2002); (g) Aloisi et al. (2007); (h) Schulte-Ladbeck et al. (2001); (i) Lelli et al. (2013); (j) Swaters & Balcells (2002); (k) Meurer et al. (1994); (l) Papaderos et al. (2002); (m) Elson et al. (2010); (n) Lelli et al. (2012b); (o) Lelli et al. (2012a).
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