Open Access
Table A.1.
ROXY best-fit parameters of the structural relations of different galaxy populations.
| Mbar − R50, bar | Mbar − Σ50, bar | R50, bar − Σ50, bar | |||||||
|---|---|---|---|---|---|---|---|---|---|
| α | β | σobs | α | β | σobs | α | β | σobs | |
| Es | ![]() |
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| bulges | ![]() |
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| Es + bulges | ![]() |
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| S0 disks | ![]() |
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| dEs/dSphs | ![]() |
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| UDGs | ![]() |
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| dEs/dSphs/UDGs | ![]() |
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| dEs(N) | ![]() |
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| Baryonic HSD disks | ![]() |
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| Stellar HSD disks | ![]() |
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| Baryonic LSD disks | ![]() |
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| Stellar LSD disks | ![]() |
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Notes. For passive galaxies, the stellar scaling relations are virtually equivalent to the baryonic ones.
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