Open Access
Table 5.
Percentages of paired galaxies that have efficient star formation and a young stellar population selected according to star mass and concentration in the void interior, void walls, and field. Standard errors are included.
| Regions | Restrictions | log(SFR/M*)> − 10.6 | Dn(4000)< 1.6 |
|---|---|---|---|
| % Void interior | log10(M*/Msun)< 9.5 | 100. ± 20.% | 100. ± 20.% |
| % Void walls | log10(M*/Msun)< 9.5 | 93. ± 9.% | 91. ± 9.% |
| % Field | log10(M*/Msun)< 9.5 | 82. ± 2.% | 83. ± 2.% |
| % Void interior | log10(M*/Msun)> 9.5 | 60. ± 6.% | 52. ± 5.% |
| % Void walls | log10(M*/Msun)> 9.5 | 50. ± 2.% | 44. ± 2.% |
| % Field | log10(M*/Msun)> 9.5 | 38.9 ± 0.8% | 32.8 ± 0.7% |
| % Void interior | C < 2.5 | 89. ± 12.% | 89. ± 12.% |
| % Void walls | C < 2.5 | 82. ± 5.% | 75. ± 4.% |
| % Field | C < 2.5 | 76. ± 1.% | 70. ± 1.% |
| % Void interior | C > 2.5 | 49. ± 6.% | 36. ± 4.% |
| % Void walls | C > 2.5 | 32. ± 2.% | 27. ± 1.% |
| % Field | C > 2.5 | 21.6 ± 0.6% | 17.1 ± 0.5% |
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