Table 2.
Main bars, [OIII]λ5007 emission, and stellar disk inclination.
| Galaxy | PAbar | Rbar | Ref. | PA[OIII] | Ref. | Open. angle | Ref. | idisk | PAdisk | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|
| (°) | (″) | (°) | (°) | (°) | (°) | |||||
| Mrk 1066 | 143 | 15.5 | 1 | 139 | 2 | 25 | 2 | 50 | 300 | 3 |
| NGC 2273 | 108 | 27 | 4 | 90 | 5 | 32 | 6 | 51 | 53 | 7 |
| NGC 4253 | 108 | ∼8 | 8 | 160 | 9 | 110 | 9 | 18 | 246 | 3 |
| NGC 4388 | 100 | 19 d | 10 | ∼35 (N) | 9 | ∼50 | 9 | 78 | 90 | 11 |
| 193 (S) | 9 | 92 | 9 | |||||||
| NGC 7465 | * | * | * | 135 | 5 | 56 | 6 | ∼60 | ∼120–130 | 12 |
Notes. Column (1) Galaxy name, Cols. (2)–(4) PA of the major axis of the main bar, radius, and reference, Cols. (4)–(5) PA of the biconical outflow inferred from the [OIII] emission and reference, Cols. (6)–(7) cone opening and reference, Cols. (8)–10) stellar galaxy disk PA, inclination and reference. The d in the radius of the bar of NGC 4388 denotes that the value is deprojected. *For the PA of the major axis of the main bar of NGC 7465, its radius and the references, see the discussion in Sect. 4.5.
References. (1) Afanasiev et al. (1998); (2) Fischer et al. (2013); (3) Riffel et al. (2017); (4) Moiseev et al. (2004); (5) Ferruit et al. (2000); (6) Our own measurements using the images in (5); (7) Barbosa et al. (2006); (8) Alonso-Herrero et al. (1998); (9) Mulchaey et al. (1996a); (10) Veilleux et al. (1999a); (11) Greene et al. (2014); (12) Merkulova et al. (2012).
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.