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Table 1.

Radiative properties of our sample of high velocity collisions at 1 d.

Model Lbol,1 d MUVW1,1 d MV,1 d VHα,1 d
[erg] [mag] [mag] [km s−1]
ms1/ms0p9/vrel5/b0p1 2.17(41) −15.3 −13.4 12 965
ms1/ms0p9/vrel5/b0p25 5.14(40) −13.5 −12.4 10 537
ms1/ms0p9/vrel2p5/b0p1 3.82(40) −13.1 −12.1 9482
ms1/ms0p9/vrel10/b0p1 5.10(41) −16.2 −14.3 20 267
ms1/ms0p9/vrel10/b0p5 9.73(40) −14.4 −12.8 11 231

ms3/ms2p7/vrel5/b0p1 2.35(41) −15.4 −13.4 13 235
ms3/ms2p7/vrel5/b0p25 7.25(40) −14.1 −12.5 10 510
ms3/ms2p7/vrel2p5/b0p1 6.55(40) −14.0 −12.4 9336
ms3/ms2p7/vrel10/b0p1 1.06(42) −16.7 −14.6 20 692
ms3/ms2p7/vrel10/b0p5 1.62(41) −15.0 −12.9 11 184

ms10/ms9/vrel5/b0p1 7.04(41) −16.2 −14.0 15 465
ms10/ms9/vrel5/b0p25 2.20(41) −15.2 −13.1 10 970
ms10/ms9/vrel5/b0p5 7.27(40) −14.1 −12.2 7637
ms10/ms9/vrel2p5/b0p1 1.93(41) −15.1 −13.1 10 794
ms10/ms9/vrel10/b0p1 3.33(42) −17.6 −15.3 9796
ms10/ms9/vrel10/b0p5 5.54(41) −15.9 −13.6 13 353

ms3/ms1/vrel5/b0p1 1.73(41) −15.1 −13.2 12 395
ms3/ms1/vrel5/b0p25 1.27(41) −14.7 −12.9 10 868
ms3/ms1/vrel5/b0p5 1.71(40) −11.8 −11.5 9181
ms3/ms1/vrel2p5/b0p1 3.72(40) −13.2 −12.0 8240
ms3/ms1/vrel2p5/b0p5 4.97(39) −9.7 −10.5 6096
ms3/ms1/vrel10/b0p1 8.08(41) −16.5 −14.4 19 141
ms3/ms1/vrel10/b0p5 7.71(40) −13.9 −12.6 12 740

ms10/ms1/vrel5/b0p1 9.00(40) −14.4 −12.6 9732
ms10/ms1/vrel5/b0p25 9.86(40) −14.5 −12.6 9805
ms10/ms1/vrel5/b0p5 3.01(40) −12.7 −11.9 9439
ms10/ms1/relv2p5/b0p1 3.11(40) −13.1 −11.7 6138
ms10/ms1/vrel2p5/b0p5 1.29(40) −11.8 −11.1 6212
ms10/ms1/vrel10/b0p1 2.94(41) −15.6 −13.6 14 728
ms10/ms1/vrel10/b0p5 1.06(41) −14.3 −12.9 14 374

ms10/ms3/vrel5/b0p1 5.60(41) −16.0 −13.8 14 134
ms10/ms3/vrel5/b0p25 4.29(41) −15.7 −13.5 12 579
ms10/ms3/vrel2p5/b0p1 1.24(41) −14.7 −12.7 8995
ms10/ms3/vrel10/b0p1 2.64(42) −17.4 −15.1 23 420
ms10/ms3/vrel10/b0p5 5.34(41) −15.9 −13.7 13 964

Notes. The table gives results from the radiative transfer calculations with CMFGEN. The columns give the model name, the bolometric luminosity, the UVW1-band and V-band magnitudes and the Doppler velocity at maximum absorption measured in the Hα line profile, all given at one day after the onset of the collision. The model name in the first column consists of the masses of the two colliding stars, their relative velocity, and the impact parameter at collision. Numbers appearing within parentheses correspond to powers of ten.

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