Chemical and Photometric Evolution Models for Disk, Irregular, and Low Mass Galaxies

Table 1

Theoretical galaxy models selected to represent a simulated Hubble sequence.

dis	𝑉max	𝑀gal	Ropt	𝜏𝑐	𝑛𝑡	𝜖𝜂	𝜖𝛿
	Km s^−1	10^11 M⊙	kpc	Gyr
3	48	0.3	2.3	31.6	8	0.037	2.6 10^−4
10	78	1.3	4.1	15.5	7	0.075	1.5 10^−3
21	122	4.3	7.1	8.1	6	0.15	1.0 10^−2
24	163	9.8	10.1	5.4	5	0.30	5.0 10^−2
28	200	17.9	13.0	4.0	4	0.45	1.4 10^−1
35	250	33.5	16.9	2.9	3	0.65	3.4 10^−1
39	290	52.7	20.6	2.3	1	0.95	8.8 10^−1