The metal to-hydrogen ratio in F1-F5 stars, as determined by a model-atmosphere analysis of photoelectric observations of a group of weak metal lines
| Image |  |
|---|---|
| Description | scientific article |
| Author/s |
author: Bengt Gustafsson |
| Publication date | 1972 |
| Language | English |
| Country of origin | |
| Wikipedia link | |
| Copyright status | |
| Missing/wrong data? | Edit Wikidata item |