The Local Bubble: a magnetic veil to our Galaxy
The magnetic field in the local interstellar medium does not follow the large-scale Galactic magnetic field. The local magnetic field has probably been distorted by the Local Bubble, a cavity of hot ionized gas extending all around the Sun and surrounded by a shell of cold neutral gas and dust. Howe...
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creator | Alves, M. I. R. Boulanger, F. Ferrière, K. Montier, L. |
description | The magnetic field in the local interstellar medium does not follow the large-scale Galactic magnetic field. The local magnetic field has probably been distorted by the Local Bubble, a cavity of hot ionized gas extending all around the Sun and surrounded by a shell of cold neutral gas and dust. However, so far no conclusive association between the local magnetic field and the Local Bubble has been established. Here we develop an analytical model for the magnetic field in the shell of the Local Bubble, which we represent as an inclined spheroid, off-centred from the Sun. We fit the model to Planck dust polarized emission observations within 30° of the Galactic poles. We find a solution that is consistent with a highly deformed magnetic field, with significantly different directions towards the north and south Galactic poles. This work sets a methodological framework for modelling the three-dimensional (3D) structure of the magnetic field in the local interstellar medium, which is a most awaited input for large-scale Galactic magnetic field models. |
doi_str_mv | 10.1051/0004-6361/201832637 |
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We find a solution that is consistent with a highly deformed magnetic field, with significantly different directions towards the north and south Galactic poles. 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R.</creatorcontrib><creatorcontrib>Boulanger, F.</creatorcontrib><creatorcontrib>Ferrière, K.</creatorcontrib><creatorcontrib>Montier, L.</creatorcontrib><title>The Local Bubble: a magnetic veil to our Galaxy</title><title>Astronomy and astrophysics (Berlin)</title><description>The magnetic field in the local interstellar medium does not follow the large-scale Galactic magnetic field. The local magnetic field has probably been distorted by the Local Bubble, a cavity of hot ionized gas extending all around the Sun and surrounded by a shell of cold neutral gas and dust. However, so far no conclusive association between the local magnetic field and the Local Bubble has been established. Here we develop an analytical model for the magnetic field in the shell of the Local Bubble, which we represent as an inclined spheroid, off-centred from the Sun. We fit the model to Planck dust polarized emission observations within 30° of the Galactic poles. We find a solution that is consistent with a highly deformed magnetic field, with significantly different directions towards the north and south Galactic poles. 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R.</creatorcontrib><creatorcontrib>Boulanger, F.</creatorcontrib><creatorcontrib>Ferrière, K.</creatorcontrib><creatorcontrib>Montier, L.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Alves, M. I. 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source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
subjects | Astronomical models Astrophysics Bubbles Cosmic dust Deformation Dust Galaxies Interstellar matter ISM: bubbles ISM: individual objects: Local Bubble ISM: magnetic fields Local interstellar medium Magnetic fields Magnetism Milky Way Neutral gases Physics Poles Three dimensional models |
title | The Local Bubble: a magnetic veil to our Galaxy |
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