Interstellar Dust and Gas in the Heliosphere
Abstract Interstellar dust and gas that enter the heliosphere provide us with important clues about both the heliosphere and the local interstellar medium (LISM). The picture we have of the LIC from both in situ detections and absorption line data presents questions that have important implications...
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crioppubl:10.1088/1742-6596/1620/1/012019 2024-06-02T07:56:33+00:00 Interstellar Dust and Gas in the Heliosphere Slavin, Jonathan 2020 http://dx.doi.org/10.1088/1742-6596/1620/1/012019 https://iopscience.iop.org/article/10.1088/1742-6596/1620/1/012019/pdf https://iopscience.iop.org/article/10.1088/1742-6596/1620/1/012019 unknown IOP Publishing http://creativecommons.org/licenses/by/3.0/ https://iopscience.iop.org/info/page/text-and-data-mining Journal of Physics: Conference Series volume 1620, issue 1, page 012019 ISSN 1742-6588 1742-6596 journal-article 2020 crioppubl https://doi.org/10.1088/1742-6596/1620/1/012019 2024-05-07T14:01:00Z Abstract Interstellar dust and gas that enter the heliosphere provide us with important clues about both the heliosphere and the local interstellar medium (LISM). The picture we have of the LIC from both in situ detections and absorption line data presents questions that have important implications for the origins and evolution of the cloud. New detections of 60 Fe on Earth in deep sea crusts and Antarctic snow cores provide evidence for the role of supernovae in shaping the LISM. We discuss our models for the evolution of the LIC inside the Local Bubble and possible explanations for the source of the supernova produced dust. Article in Journal/Newspaper Antarc* Antarctic IOP Publishing Antarctic Journal of Physics: Conference Series 1620 1 012019 |
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Abstract Interstellar dust and gas that enter the heliosphere provide us with important clues about both the heliosphere and the local interstellar medium (LISM). The picture we have of the LIC from both in situ detections and absorption line data presents questions that have important implications for the origins and evolution of the cloud. New detections of 60 Fe on Earth in deep sea crusts and Antarctic snow cores provide evidence for the role of supernovae in shaping the LISM. We discuss our models for the evolution of the LIC inside the Local Bubble and possible explanations for the source of the supernova produced dust. |
format |
Article in Journal/Newspaper |
author |
Slavin, Jonathan |
spellingShingle |
Slavin, Jonathan Interstellar Dust and Gas in the Heliosphere |
author_facet |
Slavin, Jonathan |
author_sort |
Slavin, Jonathan |
title |
Interstellar Dust and Gas in the Heliosphere |
title_short |
Interstellar Dust and Gas in the Heliosphere |
title_full |
Interstellar Dust and Gas in the Heliosphere |
title_fullStr |
Interstellar Dust and Gas in the Heliosphere |
title_full_unstemmed |
Interstellar Dust and Gas in the Heliosphere |
title_sort |
interstellar dust and gas in the heliosphere |
publisher |
IOP Publishing |
publishDate |
2020 |
url |
http://dx.doi.org/10.1088/1742-6596/1620/1/012019 https://iopscience.iop.org/article/10.1088/1742-6596/1620/1/012019/pdf https://iopscience.iop.org/article/10.1088/1742-6596/1620/1/012019 |
geographic |
Antarctic |
geographic_facet |
Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
Journal of Physics: Conference Series volume 1620, issue 1, page 012019 ISSN 1742-6588 1742-6596 |
op_rights |
http://creativecommons.org/licenses/by/3.0/ https://iopscience.iop.org/info/page/text-and-data-mining |
op_doi |
https://doi.org/10.1088/1742-6596/1620/1/012019 |
container_title |
Journal of Physics: Conference Series |
container_volume |
1620 |
container_issue |
1 |
container_start_page |
012019 |
_version_ |
1800756831488835584 |