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Table A.4.
Values of observable quantities for models of stellar populations including stripped stars and at Z = 0.0002.
| 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 = 0.0002) | |||||||||
| 2 | 52.8 {−} (52.8) | 52.2 {−} (52.2) | 48.6 {−} (48.6) | 25.9 (25.9) | 25.3 (25.3) | 21.7 (21.7) | 26.9 (26.9) | −2.0 (−2.0) | −3.08 (−3.08) |
| 3 | 52.6 {−} (52.6) | 52.0 {−} (52.0) | 47.8 {−} (47.8) | 25.5 (25.5) | 24.8 (24.8) | 20.7 (20.7) | 27.1 (27.1) | −2.0 (−2.0) | −2.77 (−2.77) |
| 5 | 52.0 {−} (52.0) | 50.9 {−} (50.9) | 45.8 {−} (45.8) | 25.2 (25.2) | 24.1 (24.1) | 19.0 (19.0) | 26.8 (26.8) | −2.2 (−2.2) | −2.61 (−2.61) |
| 7 | 51.4 {−} (51.4) | 49.6 {−} (49.6) | 40.1 {−} (40.1) | 24.7 (24.7) | 23.0 (23.0) | 13.4 (13.4) | 26.7 (26.7) | −2.4 (−2.4) | −2.57 (−2.57) |
| 11 | 50.6 {50.4} (50.2) | 49.6 {49.6} (47.3) | 44.8 {44.8} (37.2) | 24.2 (23.8) | 23.2 (20.9) | 18.5 (10.8) | 26.4 (26.4) | −2.7 (−2.8) | −2.51 (−2.5) |
| 20 | 50.5 {50.5} (49.0) | 50.0 {50.0} (45.1) | 45.4 {45.4} (−) | 24.5 (23.0) | 24.0 (19.1) | 19.4 (−) | 26.0 (26.0) | −2.7 (−3.2) | −2.42 (−2.39) |
| 30 | 50.2 {50.1} (48.4) | 49.7 {49.7} (43.9) | 44.8 {44.8} (−) | 24.3 (22.6) | 23.8 (18.1) | 19.0 (−) | 25.8 (25.8) | −2.8 (−3.4) | −2.35 (−2.32) |
| 50 | 49.6 {49.6} (47.6) | 49.0 {49.0} (42.1) | 44.0 {44.0} (−) | 24.1 (22.1) | 23.5 (16.6) | 18.4 (−) | 25.5 (25.5) | −3.0 (−3.7) | −2.15 (−2.13) |
| 100 | 49.1 {49.1} (46.4) | 48.2 {48.2} (40.5) | 42.8 {42.8} (−) | 23.9 (21.3) | 23.1 (15.3) | 17.7 (−) | 25.1 (25.1) | −3.2 (−4.1) | −1.88 (−1.85) |
| 200 | 48.2 {48.2} (45.1) | 46.8 {46.8} (38.8) | 41.3 {41.3} (−) | 23.5 (20.4) | 22.1 (14.1) | 16.5 (−) | 24.7 (24.7) | −3.5 (−4.5) | −1.57 (−1.53) |
| 300 | 47.2 {47.2} (44.3) | 45.4 {45.4} (37.0) | 40.2 {40.2} (−) | 22.7 (19.8) | 21.0 (12.6) | 15.7 (−) | 24.5 (24.5) | −3.8 (−4.8) | −1.34 (−1.3) |
| 500 | 46.3 {46.3} (43.3) | 45.0 {45.0} (−) | 40.2 {40.2} (−) | 22.1 (19.2) | 20.9 (−) | 16.1 (−) | 24.1 (24.1) | −4.1 (−5.1) | −0.96 (−0.91) |
| 800 | 44.8 {44.8} (42.0) | 42.0 {42.0} (−) | 35.6 {35.6} (−) | 21.2 (18.3) | 18.3 (−) | 11.9 (−) | 23.7 (23.6) | −4.6 (−5.6) | 0.06 (0.14) |
| 1000 | 41.4 {−} (41.4) | − {−} (−) | − {−} (−) | 18.0 (18.0) | − (−) | − (−) | 23.4 (23.4) | −5.8 (−5.8) | 1.03 (1.03) |
| Continuous star-formation (1 M⊙/year, Z = 0.0002) | |||||||||
| 500 | 53.3 {52.0} (53.3) | 52.7 {51.4} (52.6) | 48.9 {46.8} (48.9) | 25.2 (25.2) | 24.6 (24.6) | 20.8 (20.8) | 28.1 (28.1) | −1.8 (−1.8) | −2.39 (−2.38) |
Notes. This table is analogous to Table 1, but for a population of stripped stars with Z = 0.0002. We compare to the STARBURST99 models with Z = 0.001.
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