Some papers have been devoted to the study of chemical abundances in CP stars. Below you can find some examples of such activities.
In the paper:
High resolution spectroscopy
of HD207538 from Far-UV (FUSE) to visible (SARG-TNG).
A global picture of the stellar and
interstellar features modeled.
G. Catanzaro,
M. K. André, F. Leone, P. Sonnentrucker
2003,
Astronomy and Astrophysics, 404, 677
we pointed our attention on the modeling of the stellar spectrum in a wide spectral range, namely from Far-UV to visible, giving a global description of the stellar and interstellar features observed. Following figures were extracted from that paper.
| Modeling of ISM and stellar lines in the FUSE range 1000 - 1090 Angstrom | Modeling of ISM and stellar lines in the FUSE range 1090 - 1190 Angstrom | Modeling of stellar lines in the TNG-SARG range 4630 - 5750 Angstrom | Modeling of ISM NAI doublet |
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HD 191110 a SB2
system with Hg and HgMn components.
Orbital elements and abundance analysis.
G. Catanzaro,
F. Leone, P. Leto
2003,
Astronomy and Astrophysics, 407, 669
we studied the SB2 system HD 191110, performing a quantitative abundance analysis of both components. We developped a method to compute simultaneously the effective temperatures and surface gravities of both components and the light ratio between them.
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Comparison between computed and observed Hb line profiles. |
Synthetic spectrum compared with the observations around l4507 Angstrom | Synthetic spectrum compared with the observations around l3984 Angstrom | Synthetic spectrum compared with the observations around l4923 Angstrom |
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click here to see the radial velocities curves of both components.
