Table 2
Sample of regions found with positive detection of WR features.
| Galaxy | Region | ΔAR | ΔDec | d/reff | r | ε | εorig | EW(Hα)obs | Hα | Class | Red |
| ID | (arcsec) | (arcsec) | (pc) | (Å) | clump | bump | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
|
|
|||||||||||
| IC 0225 | R1 | 1.7 | 0.0 | 0.0 | 346 | 10.4 | 6.3 | 121 | 1 | 1 | 0 |
| IC 0776 | R1 | 12.6 | 6.5 | 0.4 | 547 | 9.0 | 6.6 | 421 | 1 | 1 | 0 |
| NGC 0216 | R1 | −4.7 | −16.9 | 0.6 | 470 | 11.7 | 6.3 | 86 | 1 | 1 | 0 |
| R2 | −2.0 | −8.9 | 0.3 | 180 | 11.0 | 4.6 | 25 | 0 | 0 | 0 | |
| NGC 1056 | R1 | −1.7 | −3.6 | 0.3 | 554 | 9.7 | 3.8 | 53 | 1 | 0 | 0 |
| NGC 2604 | R1 | 1.8 | −0.3 | 0.0 | 421 | 13.9 | 9.0 | 139 | 1 | 1 | 0 |
| NGC 3353 | R1 | −0.5 | 0.7 | 0.1 | 372 | 29.1 | 11.7 | 317 | 1 | 1 | 1 |
| NGC 3381 | R1 | −0.8 | −0.4 | 0.0 | 365 | 31.2 | 10.5 | 115 | 1 | 1 | 0 |
| NGC 3773 | R1 | 2.3 | −0.4 | 0.0 | 237 | 24.0 | 11.8 | 148 | 1 | 1 | 1 |
| NGC 3991 | R1 | −1.0 | −6.7 | 0.4 | 956 | 13.0 | 5.9 | 154 | 1 | 1 | 1 |
| R2 | 1.8 | 0.8 | 0.1 | 750 | 17.0 | 8.4 | 229 | 1 | 1 | 1 | |
| NGC 3994 | R1 | 1.0 | −7.8 | 0.8 | 428 | 10.2 | 5.5 | 109 | 1 | 1 | 0 |
| R2 | −5.4 | −7.2 | 1.0 | 343 | 8.6 | 4.4 | 57 | 1 | 0 | 0 | |
| R3 | −0.1 | 7.9 | 0.8 | 343 | 7.8 | 4.2 | 66 | 1 | 0 | 0 | |
| NGC 4470 | R1 | 6.4 | −10.0 | 0.8 | 482 | 11.3 | 5.0 | 26 | 1 | 1 | 0 |
| R2 | 11.8 | −3.8 | 0.8 | 519 | 9.8 | 5.0 | 58 | 1 | 1 | 0 | |
| R3 | 1.3 | 10.9 | 0.7 | 432 | 9.5 | 4.2 | 68 | 1 | 0 | 0 | |
| NGC 4630 | R1 | −1.2 | −0.2 | 0.0 | 133 | 14.1 | 6.7 | 168 | 1 | 1 | 0 |
| NGC 5145 | R1 | 8.2 | −0.3 | 0.6 | 172 | 9.4 | 4.6 | 54 | 0 | 0 | 0 |
| NGC 5630 | R1 | −10.0 | 3.8 | 0.4 | 849 | 8.8 | 5.4 | 72 | 1 | 1 | 0 |
| NGC 5665 | R1 | 5.0 | −6.0 | 0.4 | 262 | 10.1 | 4.0 | 46 | 0 | 0 | 0 |
| R2 | 6.9 | −1.0 | 0.3 | 468 | 11.7 | 5.2 | 125 | 1 | 1 | 0 | |
| R3 | 24.4 | −1.1 | 1.2 | 556 | 16.6 | 11.3 | 192 | 1 | 1 | 0 | |
| R4 | −3.5 | −0.9 | 0.2 | 262 | 11.1 | 4.4 | 38 | 0 | 0 | 0 | |
| R5 | −5.9 | 2.5 | 0.3 | 468 | 8.6 | 4.3 | 48 | 1 | 0 | 0 | |
| R6 | 8.1 | 4.1 | 0.4 | 504 | 15.6 | 7.1 | 219 | 1 | 1 | 0 | |
| R7 | −3.5 | 8.8 | 0.5 | 476 | 8.8 | 4.9 | 58 | 1 | 0 | 0 | |
| R8 | 7.2 | 9.8 | 0.6 | 461 | 9.9 | 4.8 | 101 | 1 | 0 | 0 | |
| NGC 5953 | R1 | 0.5 | −6.2 | 0.4 | 268 | 9.1 | 3.9 | 74 | 0 | 0 | 0 |
| NGC 5954 | R1 | 0.7 | 0.9 | 0.1 | 372 | 9.3 | 3.9 | 74 | 1 | 0 | 0 |
| R2 | 4.9 | 2.4 | 0.4 | 398 | 9.9 | 5.4 | 148 | 1 | 1 | 0 | |
| R3 | 5.4 | 10.5 | 0.9 | 423 | 10.7 | 6.7 | 279 | 1 | 1 | 0 | |
| NGC 6090 | R1 | 0.2 | −1.3 | 0.0 | 1915 | 16.2 | 8.9 | 51 | 1 | 1 | 0 |
| NGC 7469 | R1 | 1.1 | −0.7 | 0.0 | 1306 | 10.0 | 8.9 | 67 | 1 | 1 | 0 |
| UGC 00312 | R1 | −3.9 | −23.1 | 1.3 | 958 | 7.8 | 6.4 | 371 | 1 | 1 | 0 |
| R2 | −0.7 | −7.2 | 0.4 | 932 | 8.5 | 7.7 | 109 | 1 | 1 | 0 | |
| R3 | 2.3 | −1.2 | 0.1 | 848 | 7.0 | 3.8 | 83 | 1 | 0 | 0 | |
| UGC 10297 | R1 | −1.1 | 16.2 | 0.6 | 432 | 8.7 | 6.9 | 231 | 1 | 1 | 0 |
| UGC 10331 | R1 | 2.5 | −2.0 | 0.1 | 1107 | 8.8 | 5.4 | 161 | 1 | 1 | 0 |
| R2 | −4.3 | 0.8 | 0.2 | 1082 | 10.7 | 6.4 | 137 | 1 | 1 | 0 | |
| UGC 10650 | R1 | 0.3 | −0.9 | 0.1 | 669 | 13.0 | 8.5 | 165 | 1 | 1 | 0 |
| UGC 6320 | R1 | 1.7 | −0.3 | 0.1 | 295 | 29.1 | 12.4 | 256 | 1 | 1 | 1 |
| R2 | 1.1 | −6.5 | 0.2 | 284 | 9.4 | 6.1 | 216 | 1 | 1 | 0 | |
| UGC 9663 | R1 | 15.1 | 8.4 | 0.6 | 598 | 10.0 | 7.6 | 699 | 1 | 1 | 0 |
Notes. Column (1): name of the galaxy. Column (2): region identification number. Column (3): offset in Right Ascension from the centre of the galaxy. Column (4): offset in declination from the centre of the galaxy. Column (5): projected distance to the centre of the galaxy, normalised to the effective radius. Column (6): radius of the associated Hα clump (if not possible association, radius of the region), derived as 
, where A corresponds to the number of pixels that form the region (note that each pixel represent an area of 1 arcsec2). Column (7): ε for the integrated spectrum of the region, after the subtracting the underlying stellar emission with STARLIGHT (see text). Column (8): same as (7), but for the observed integrated spectrum. Column (9): Hα equivalent width of the observed integrated spectrum. Column (10): flag indicating whether a given region belongs to an Hα clump (1) or to the more extended Hα emission of the galaxy (0). Column (11): adopted class for the detection significance of the WR features in the regions. Column(12): flag indicating if the red bump is detected (1) or not (0).
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.