The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion
We describe the interface between the outer heliosphere and the local interstellar medium (LISM) surrounding the Sun. The components of the inner LISM are the four partially ionized clouds [the Local Interstellar Cloud (LIC), G cloud, Blue cloud, and Aql cloud] that are in contact with the outer hel...
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ftdatacite:10.48550/arxiv.1910.01243 2023-05-15T13:59:58+02:00 The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion Linsky, Jeffrey L. Redfield, Seth Tilipman, Dennis 2019 https://dx.doi.org/10.48550/arxiv.1910.01243 https://arxiv.org/abs/1910.01243 unknown arXiv https://dx.doi.org/10.3847/1538-4357/ab498a arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Solar and Stellar Astrophysics astro-ph.SR Astrophysics of Galaxies astro-ph.GA FOS Physical sciences article-journal Article ScholarlyArticle Text 2019 ftdatacite https://doi.org/10.48550/arxiv.1910.01243 https://doi.org/10.3847/1538-4357/ab498a 2022-03-10T16:15:10Z We describe the interface between the outer heliosphere and the local interstellar medium (LISM) surrounding the Sun. The components of the inner LISM are the four partially ionized clouds [the Local Interstellar Cloud (LIC), G cloud, Blue cloud, and Aql cloud] that are in contact with the outer heliosphere, and ionized gas produced by EUV radiation primarily from $ε$~CMa. We construct the three-dimensional shape of the LIC based on interstellar line absorption along 62 sightlines and show that in the direction of $ε$~CMa, $β$~CMa, and Sirius~B the neutral hydrogen column density from the center of the LIC is a minimum. We call this region the ``hydrogen hole''. In this direction, the presence of Blue cloud absorption and the absence of LIC absorption can be simply explained by the Blue cloud lying just outside of the heliosphere. We propose that the outer edge of the Blue cloud is a Strömgren shell driven toward the heliosphere by high pressures in the H~II region. We find that the vectors of neutral and ionized helium flowing through the heliosphere are inconsistent with the LIC flow vector, and that the nearby intercloud gas is consistent with ionization by $ε$~CMa and other stellar sources without requiring additional sources of ionization or million degree plasma. In the upwind direction, the heliosphere is passing through an environment of several LISM clouds, which may explain the recent influx of interstellar grains containing $^{60}$Fe from supernova ejecta measured in Antarctica snow. : 52 pages, 11 figures, to appear in the Astrophysical Journal Article in Journal/Newspaper Antarc* Antarctica DataCite Metadata Store (German National Library of Science and Technology) Sirius ENVELOPE(163.250,163.250,-84.133,-84.133) |
institution |
Open Polar |
collection |
DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
unknown |
topic |
Solar and Stellar Astrophysics astro-ph.SR Astrophysics of Galaxies astro-ph.GA FOS Physical sciences |
spellingShingle |
Solar and Stellar Astrophysics astro-ph.SR Astrophysics of Galaxies astro-ph.GA FOS Physical sciences Linsky, Jeffrey L. Redfield, Seth Tilipman, Dennis The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion |
topic_facet |
Solar and Stellar Astrophysics astro-ph.SR Astrophysics of Galaxies astro-ph.GA FOS Physical sciences |
description |
We describe the interface between the outer heliosphere and the local interstellar medium (LISM) surrounding the Sun. The components of the inner LISM are the four partially ionized clouds [the Local Interstellar Cloud (LIC), G cloud, Blue cloud, and Aql cloud] that are in contact with the outer heliosphere, and ionized gas produced by EUV radiation primarily from $ε$~CMa. We construct the three-dimensional shape of the LIC based on interstellar line absorption along 62 sightlines and show that in the direction of $ε$~CMa, $β$~CMa, and Sirius~B the neutral hydrogen column density from the center of the LIC is a minimum. We call this region the ``hydrogen hole''. In this direction, the presence of Blue cloud absorption and the absence of LIC absorption can be simply explained by the Blue cloud lying just outside of the heliosphere. We propose that the outer edge of the Blue cloud is a Strömgren shell driven toward the heliosphere by high pressures in the H~II region. We find that the vectors of neutral and ionized helium flowing through the heliosphere are inconsistent with the LIC flow vector, and that the nearby intercloud gas is consistent with ionization by $ε$~CMa and other stellar sources without requiring additional sources of ionization or million degree plasma. In the upwind direction, the heliosphere is passing through an environment of several LISM clouds, which may explain the recent influx of interstellar grains containing $^{60}$Fe from supernova ejecta measured in Antarctica snow. : 52 pages, 11 figures, to appear in the Astrophysical Journal |
format |
Article in Journal/Newspaper |
author |
Linsky, Jeffrey L. Redfield, Seth Tilipman, Dennis |
author_facet |
Linsky, Jeffrey L. Redfield, Seth Tilipman, Dennis |
author_sort |
Linsky, Jeffrey L. |
title |
The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion |
title_short |
The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion |
title_full |
The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion |
title_fullStr |
The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion |
title_full_unstemmed |
The interface between the outer heliosphere and the inner lism: Morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$Fe accretion |
title_sort |
interface between the outer heliosphere and the inner lism: morphology of the local interstellar cloud, its hydrogen hole, stromgren shells, and $^{60}$fe accretion |
publisher |
arXiv |
publishDate |
2019 |
url |
https://dx.doi.org/10.48550/arxiv.1910.01243 https://arxiv.org/abs/1910.01243 |
long_lat |
ENVELOPE(163.250,163.250,-84.133,-84.133) |
geographic |
Sirius |
geographic_facet |
Sirius |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
https://dx.doi.org/10.3847/1538-4357/ab498a |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1910.01243 https://doi.org/10.3847/1538-4357/ab498a |
_version_ |
1766268878455832576 |