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Table 2

Trends of NSG/NTOT ratios.

Parameter TF TuF
N NSG/NTOT ≈, M ↑s, tdisss NSG/NTOT ≈, M ↑, tdisss
rg NSG/NTOT ≈, M ↑s, tdiss NSG/NTOT ≈, M ↑s, tdiss
fb NSG/NTOTw, M ↑w, tdisss NSG/NTOT ≈, M ≈, tdiss
Mmax NSG/NTOT ↓, M ≈, tdiss NSG/NTOT ≈, M ≈, tdiss
concpop NSG/NTOT ↓, M ≈, tdiss NSG/NTOT ≈, M ↑w, tdiss
W0,FG NSG/NTOTs, M ↑s, tdisss NSG/NTOT ≈, M ≈, tdiss
rhFG NSG/NTOT ↑, M ↓, tdiss
Parameter TF TuF
tdiss N ↑s, rg ↑, W0,FGs, Mmax N ↑s
NSG/NTOT fb↑w rhFG
M↑ N ↑s, rgs, fb ↑, W0,FGs N ↑, rgs

Notes. Top table summarizes how by increasing one parameter (Col. 1) one can influence NSG/NTOT ratios, total GC mass (M), and time of dissolution (tdiss) of GC for both tidally filling (TF, Col. 2) and tidally underfilling models (TuF, Col. 3). The arrows show whether a given parameter is increasing (↑), decreasing (↓), particularly strong (↑s, ↓s), or weak (↑w, ↓w). The bottom table shows the same, but from the point of view of the GC global parameters, whose initial parameters one has to increase to get higher NSG/NTOT, M, or tdiss values (up to Hubble time).

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