Table A.4.
Morphological features detected visually in the photometric images of the 96 relaxed S0-like remnants.
No. | Model | Morph. Type | Merger-related features | Bar? | Global features | Tidal satellites? |
---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) |
1 | gE0gSao1 | S0 | – | – | SL (oval), NB | Y |
2 | gE0gSao5 | S0 | Plume | – | SL, ISp | – |
3 | gE0gSao16 | S0 | – | – | SL | – |
4 | gE0gSao44 | S0 | – | – | LL | – |
5 | gE0gSbo5 | S0 | – | – | SL | – |
6 | gE0gSbo44 | S0 | Plume | – | SL | – |
… | … | … | … | … | … | … |
Notes. Column 1: ordering number. Column 2: model ID. Column 3: visual morphological type. Column 4: morphological features detected in the photometric images of the remnant indicating past merger activity. Used acronyms: “DA”: disc asymmetry; “TD”: tidal debris; “TT”: tidal tail. Column 5: whether the final remnant is barred (“Y”) or not (“–”). Column 6: relevant morphological features detected in the photometric images of the remnant, not necessarily related to a merger origin. Used acronyms: “FL”: flat lens; “ID”: inner disc; “IID”: inclined inner disc; “IPR”: inner pseudo-ring; “IR”: inner ring; “ISp”: inner spiral; “LL”: lentil-shaped lens; “NB”: nuclear bar; “OR”: outer ring; “OSR”: outer spiral relics; “SL”: spheroidal lens. Column 7: whether there are tidal satellites orbiting the remnant within a FoV of 100 × 100 kpc2 for the face-on and edge-on views (“Y”: there is at least one; “–”: none). A full version of this Table is available at the CDS.
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