|
par1 | , surface (unredshifted) effective temperature |
par2 | , neutron star gravitational mass |
par3 | , neutron star radius |
par4 | , distance to neutron star |
par5 | switch indicating model to use |
norm | 1, normalization (though not strictly correct, can be varied to change the size of the emission region, () |
The models available by setting par5 are:
Switch | Element | ( G) | (cm/s) | (keV) | |||
1000 | H | 0.01 | 0 | N/A | 2.4 | 5.5 – 6.7 | 0.05 – 10 |
1060 | H | 0.04 | 0 | N/A | 0.4 – 2.5 | 5.5 – 6.7 | 0.05 – 10 |
1085 | H | 0.07 | 0 | N/A | 0.4 – 2.5 | 5.5 – 6.7 | 0.05 – 10 |
1100 | H | 0.1 | 0 | N/A | 0.4 – 2.5 | 5.5 – 6.7 | 0.05 – 10 |
1170 | H | 0.5 | 0 | N/A | 0.4 – 2.5 | 5.5 – 6.8 | 0.05 – 10 |
1185 | H | 0.71 | 0 | N/A | 2.4 | 5.5 – 6.8 | 0.05 – 10 |
1195 | H | 0.89 | 0 | N/A | 2.4 | 5.5 – 6.8 | 0.05 – 10 |
1200 | H | 1.0 | 0 | N/A | 0.4 – 2.5 | 5.5 – 6.8 | 0.05 – 10 |
1230 | H | 2.0 | 0 | N/A | 2.4 | 5.5 – 6.8 | 0.05 – 10 |
1260 | H | 4.0 | 0 | N/A | 2.4 | 5.5 – 6.8 | 0.05 – 10 |
1280 | H | 7.0 | 0 | N/A | 2.4 | 5.5 – 6.8 | 0.05 – 10 |
1300 | H | 10.0 | 0 | N/A | 0.4 – 2.5 | 5.5 – 6.8 | 0.05 – 10 |
1330 | H | 20.0 | 0 | N/A | 2.4 | 5.6 – 6.8 | 0.05 – 10 |
1350 | H | 30.0 | 0 | N/A | 2.4 | 5.7 – 6.8 | 0.05 – 10 |
1211 | H | 1.26 | 0 | N/A | 1.6 | 5.5 – 6.8 | 0.05 – 10 |
1281 | H | 7.0 | 0 | N/A | 1.6 | 5.5 – 6.8 | 0.05 – 10 |
12006 | C | 1.0 | 0 | N/A | 2.4 | 5.8 – 6.9 | 0.05 – 10 |
13006 | C | 10.0 | 0 | N/A | 2.4 | 5.8 – 6.9 | 0.05 – 10 |
12008 | O | 1.0 | 0 | N/A | 2.4 | 5.8 – 6.9 | 0.05 – 10 |
13008 | O | 10.0 | 0 | N/A | 2.4 | 5.8 – 6.9 | 0.05 – 10 |
12010 | Ne | 1.0 | 0 | N/A | 2.4 | 5.8 – 6.9 | 0.05 – 10 |
13010 | Ne | 10.0 | 0 | N/A | 2.4 | 5.8 – 6.9 | 0.05 – 10 |
123100 | H | 1.0 – 1.82 | 0-90 | 0 | 1.6 | 5.5 – 6.8 | 0.09 – 5 |
123190 | H | 1.0 – 1.82 | 0-90 | 90 | 1.6 | 5.5 – 6.8 | 0.09 – 5 |
130100 | H | 5.5 – 10.0 | 0-90 | 0 | 1.6 | 5.5 – 6.8 | 0.09 – 5 |
130190 | H | 5.5 – 10.0 | 0-90 | 90 | 1.6 | 5.5 – 6.8 | 0.09 – 5 |
If you publish results obtained using nsmaxg, please reference Ho (2014).
HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public
Last modified: Friday, 23-Aug-2024 13:20:40 EDT