Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. I. ^60^Fe transport to the solar system by turbulent mixing of ejecta from nearby supernovae into a locally homogeneous interstellar medium
| Image |  |
|---|---|
| Description | scientific article |
| Author/s | |
| Publication date | 2017 |
| Language | English |
| Country of origin | |
| Wikipedia link | |
| Copyright status | |
| Missing/wrong data? | Edit Wikidata item |