Abstract
Abundances for the elements W, Os, and Bi are presented for the HgMn star chi Lupi, based upon GHRS echelle-mode spectra and a synthetic spectrum analysis. The tungsten abundance is consistent with a solar-system value while the osmium and bismuth abundances reflect enhancements. With these new data we are able to quantitatively define an abundance peak within the element range Z = 74 through 83.
| Original language | English |
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| Title of host publication | The Scientific Impact of the Goddard High Resolution Spectrograph (Astronomical Society of the Pacific Conference Series) |
| Publisher | Astronomical Society of the Pacific (ASP) |
| Pages | 330-333 |
| Volume | 143 |
| ISBN (Print) | 1-886733-63-5 |
| Publication status | Published - 1998 |
| Event | Symposium on the Scientific Impact of the Goddard High Resolution Spectrograph - Greenbelt, MD Duration: 1996 Sept 11 → 1996 Sept 12 |
Publication series
| Name | |
|---|---|
| Volume | 143 |
Conference
| Conference | Symposium on the Scientific Impact of the Goddard High Resolution Spectrograph |
|---|---|
| Period | 1996/09/11 → 1996/09/12 |
Bibliographical note
The information about affiliations in this record was updated in December 2015.The record was previously connected to the following departments: Lund Observatory (000006111), Physics, science (011013100), Science (000006100)
Subject classification (UKÄ)
- Astronomy, Astrophysics and Cosmology