Table 5.
Best-fit model parameters for a single-temperature CIE model fit to the RGS spectra of MRK 1216.
| kT (keV) | 0.73 ± 0.02 |
| s | 0.53 ± 0.04 |
| O (Solar) | 1.3 ± 0.4 |
| Ne (Solar) | 1.4 ± 0.5 |
| Mg (Solar) | 2.1 ± 0.7 |
| Fe (Solar) | 1.0 ± 0.3 |
Notes. The spectra were extracted from a 0.5′ wide region centered on MRK 1216. The scale factor s is the ratio of the observed LSF to the expected LSF based on the radial surface brightness profile extracted in the dispersion direction. The abundances are given with respect to the proto-Solar abundances of Lodders & Palme (2009).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.