Table 1
Overview of bulge classification.
ID | NED name | B/T | n b | C 20,50 | ∇σ | Kormendy rel. | Classification |
≤ 1.5 | ≥ 0.4 | ≥ −0.18 | low-outlier | ||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|||||||
2 | UGC 00005 | 0.01 | ps | ps | cl | ps | pseudo |
3 | NGC 7819 | 0.12 | ps | cl | cl | ps | |
6 | NGC 7824 | 0.38 | cl | cl | cl | cl | classical |
8 | NGC 0001 | 0.41 | cl | cl | cl | cl | classical |
20 | NGC 0160 | 0.29 | cl | cl | cl | cl | classical |
31 | NGC 0234 | 0.04 | ps | ps | ps | ps | pseudo |
33 | NGC 0257 | 0.10 | cl | cl | ps | cl | classical |
43 | IC 1683 | 0.12 | ps | cl | cl | cl | classical |
45 | NGC 0496 | bulgeless | bulgeless | ps | ps | bulgeless | bulgeless |
47 | NGC 0517 | 0.55 | cl | cl | ps | cl | classical |
119 | NGC 1167 | 0.23 | cl | cl | cl | cl | classical |
147 | NGC 2253 | 0.08 | cl | cl | cl | cl | classical |
275 | NGC 2906 | 0.14 | cl | ps | ps | ps | pseudo |
277 | NGC 2916 | 0.07 | cl | ps | cl | cl | classical |
311 | NGC 3106 | 0.30 | cl | cl | cl | cl | classical |
489 | NGC 4047 | 0.03 | cl | ps | ps | ps | pseudo |
548 | NGC 4470 | bulgeless | bulgeless | ps | ps | bulgeless | bulgeless |
580 | NGC 4711 | 0.02 | ps | ps | ps | ps | pseudo |
607 | UGC 08234 | 0.58 | cl | cl | cl | cl | classical |
611 | NGC 5016 | 0.01 | ps | ps | ps | ps | pseudo |
715 | NGC 5520 | 0.26 | ps | cl | ps | cl | |
748 | NGC 5633 | bulgeless | bulgeless | ps | ps | bulgeless | bulgeless |
768 | NGC 5732 | 0.04 | ps | ps | no data | ps | pseudo |
769 | UGC 09476 | 0.03 | ps | ps | ps | ps | pseudo |
778 | NGC 5784 | 0.39 | cl | cl | ps | cl | classical |
821 | NGC 6060 | 0.06 | ps | ps | ps | cl | pseudo |
823 | NGC 6063 | 0.01 | ps | ps | ps | ps | pseudo |
826 | NGC 6081 | 0.35 | cl | cl | cl | cl | classical |
836 | NGC 6155 | 0.01 | ps | ps | ps | ps | pseudo |
849 | NGC 6301 | 0.01 | ps | ps | cl | ps | pseudo |
850 | NGC 6314 | 0.33 | cl | cl | cl | cl | classical |
856 | IC 1256 | 0.03 | cl | ps | ps | ps | pseudo |
858 | UGC 10905 | 0.52 | cl | cl | cl | cl | classical |
874 | NGC 7025 | 0.44 | cl | cl | cl | cl | classical |
877 | UGC 11717 | 0.20 | cl | cl | no data | cl | classical |
886 | NGC 7311 | 0.32 | cl | cl | cl | cl | classical |
889 | NGC 7364 | 0.45 | cl | cl | ps | cl | classical |
891 | UGC 12224 | 0.02 | ps | ps | ps | ps | pseudo |
898 | NGC 7489 | 0.02 | ps | ps | cl | ps | pseudo |
912 | NGC 7623 | 0.49 | cl | cl | cl | cl | classical |
913 | NGC 7625 | 0.14 | ps | cl | ps | ps | pseudo |
915 | NGC 7653 | 0.27 | cl | cl | cl | cl | classical |
916 | NGC 7671 | 0.33 | cl | cl | cl | cl | classical |
917 | NGC 7683 | 0.57 | cl | cl | cl | cl | classical |
923 | NGC 7711 | 0.47 | cl | cl | cl | cl | classical |
Notes. (1) CALIFA ID; (2) NED name; (3) bulge-to-total light ratio, for reference. We list four different bulge classification criteria in Cols. 4–7: (4) bulge Sérsic index; (5) concentration index; (6) central velocity dispersion gradient; (7) Kormendy relation. (8) Final classification: in the last column we assign each bulge a final classification if and only if at least three out of four criteria are in agreement. With “pseudo” we are referring to the inner disc of galaxies built through secular evolution, as explained in more detail in the text. The second line of the head of the table shows the boundaries that we have defined to demarcate pseudobulges. If a value of a specific cell in Cols. 4–7 is within these limits it is annotated as “ps”, otherwise it is “cl”, which refers to “pseudobulge” and “classical bulge”, respectively. The 3 bulgeless galaxies are annotated in Cols. 3, 4 and 7. Two galaxies have no kinematic data, and thus no value in Col. 6.
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