Isotopic composition of Hg and Pt in slowly rotating HgMn stars
| dc.creator | Hubrig, S. | |
| dc.creator | Castelli, F. | |
| dc.creator | Mathys, G. | |
| dc.date | 1998-05-14 | |
| dc.date.accessioned | 2026-07-07T02:26:55Z | |
| dc.date.available | 2026-07-07T02:26:55Z | |
| dc.description | Preliminary results from a study of the isotopic compositions of the elements Hg and Pt in a number of HgMn stars are presented. This work represents an improvement over previous studies thanks to the very high spectral resolution available (R = 118 000) and to the new information on wavelengths and atomic structure of Hg II and Pt II. | |
| dc.description | 3 pages, no figure, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schnell and J. Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No 3 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9805189 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9805189 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12478 | |
| dc.subject | Astrophysics | |
| dc.title | Isotopic composition of Hg and Pt in slowly rotating HgMn stars | |
| dc.type | text |