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Table A.3.
Values of observable quantities for models of stellar populations including stripped stars and at Z = 0.002.
| Time | log10 Q0, pop | log10Q1, pop | log10Q2, pop | log10ξion, 0 | log10ξion, 1 | log10ξion, 2 | log10 Lν(1500 Å) | log10U | β |
|---|---|---|---|---|---|---|---|---|---|
| [Myr] | [s−1] | [s−1] | [s−1] | [erg−1 Hz] | [erg−1 Hz] | [erg−1 Hz] | [erg s−1 Hz−1] | ||
| Section | 5 | 5 | 5 | 6.1.1 | 6.1.1 | 6.1.1 | 6.1.1 | 6.1.2 | 6.2 |
| Co-eval stellar population (106 M⊙, Z = 0.002) | |||||||||
| 2 | 52.7 {−} (52.7) | 52.2 {−} (52.2) | 48.9 {−} (48.9) | 25.8 (25.8) | 25.2 (25.2) | 21.9 (21.9) | 26.9 (26.9) | −2.0 (−2.0) | −3.08 (−3.08) |
| 3 | 52.6 {−} (52.6) | 51.9 {−} (51.9) | 47.6 {−} (47.6) | 25.5 (25.5) | 24.8 (24.8) | 20.5 (20.5) | 27.1 (27.1) | −2.0 (−2.0) | −2.74 (−2.74) |
| 5 | 52.0 {−} (52.0) | 50.9 {−} (50.9) | 45.1 {−} (45.1) | 25.2 (25.2) | 24.1 (24.1) | 18.3 (18.3) | 26.8 (26.8) | −2.2 (−2.2) | −2.58 (−2.58) |
| 7 | 51.4 {−} (51.4) | 49.5 {−} (49.5) | 39.8 {−} (39.8) | 24.7 (24.7) | 22.9 (22.9) | 13.1 (13.1) | 26.7 (26.7) | −2.4 (−2.4) | −2.51 (−2.51) |
| 11 | 51.0 {50.9} (50.3) | 50.7 {50.7} (47.4) | 48.6 {48.6} (37.1) | 24.6 (23.9) | 24.3 (21.0) | 22.3 (10.7) | 26.4 (26.4) | −2.6 (−2.8) | −2.43 (−2.42) |
| 20 | 50.5 {50.4} (49.1) | 50.2 {50.2} (45.2) | 47.2 {47.2} (−) | 24.5 (23.2) | 24.2 (19.2) | 21.2 (−) | 26.0 (26.0) | −2.7 (−3.2) | −2.34 (−2.33) |
| 30 | 50.1 {50.1} (48.5) | 49.8 {49.8} (43.8) | 46.5 {46.5} (−) | 24.4 (22.7) | 24.0 (18.0) | 20.7 (−) | 25.8 (25.8) | −2.8 (−3.4) | −2.28 (−2.27) |
| 50 | 49.7 {49.7} (47.7) | 49.3 {49.3} (41.8) | 45.2 {45.2} (−) | 24.2 (22.2) | 23.8 (16.3) | 19.6 (−) | 25.5 (25.5) | −3.0 (−3.7) | −2.1 (−2.09) |
| 100 | 49.1 {49.1} (46.5) | 48.5 {48.5} (40.1) | 43.2 {43.2} (−) | 23.9 (21.3) | 23.4 (15.0) | 18.1 (−) | 25.1 (25.1) | −3.2 (−4.1) | −1.84 (−1.82) |
| 200 | 48.3 {48.3} (44.9) | 47.2 {47.2} (38.4) | 41.4 {41.4} (−) | 23.5 (20.2) | 22.4 (13.6) | 16.7 (−) | 24.7 (24.7) | −3.5 (−4.6) | −1.54 (−1.52) |
| 300 | 47.6 {47.6} (43.9) | 46.8 {46.8} (36.4) | 41.7 {41.7} (−) | 23.1 (19.5) | 22.3 (12.0) | 17.3 (−) | 24.5 (24.5) | −3.7 (−4.9) | −1.33 (−1.3) |
| 500 | 46.2 {46.2} (42.9) | 44.6 {44.6} (−) | 39.7 {39.7} (−) | 22.1 (18.8) | 20.5 (−) | 15.6 (−) | 24.1 (24.1) | −4.2 (−5.3) | −0.96 (−0.93) |
| 800 | 45.0 {45.0} (41.5) | 42.2 {42.2} (−) | 36.1 {36.1} (−) | 21.3 (17.9) | 18.6 (−) | 12.5 (−) | 23.6 (23.6) | −4.6 (−5.7) | 0.1 (0.19) |
| 1000 | 44.3 {44.3} (40.8) | 41.2 {41.2} (−) | 34.2 {34.2} (−) | 20.9 (17.5) | 17.8 (−) | 10.8 (−) | 23.4 (23.4) | −4.8 (−5.9) | 0.97 (1.11) |
| Continuous star-formation (1 M⊙/year, Z = 0.002) | |||||||||
| 500 | 53.3 {52.0} (53.3) | 52.6 {51.7} (52.6) | 49.4 {49.1} (49.1) | 25.2 (25.2) | 24.6 (24.5) | 21.3 (21.0) | 28.1 (28.1) | −1.8 (−1.8) | −2.35 (−2.35) |
Notes. This table is analogous to Table 1, but for a population of stripped stars with Z = 0.002. We compare to the STARBURST99 models with Z = 0.002.
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