Academic Journal

Constraining the magnetic field of the Smith High-velocity Cloud using Faraday rotation

التفاصيل البيبلوغرافية
العنوان: Constraining the magnetic field of the Smith High-velocity Cloud using Faraday rotation
المؤلفون: Betti, S. K., Hill, Alex S., Mao, S. A., Gaensler, B. M., Lockman, Felix J., Mcclure-Griffiths, N. M., Benjamin, Robert A.
بيانات النشر: IOP
سنة النشر: 2019
المجموعة: National Research Council Canada: NRC Publications Archive
مصطلحات موضوعية: ISM: individual objects (Smith Cloud), ISM: magnetic fields, polarization, radio continuum: general
الوصف: The Smith Cloud is a high-velocity cloud with an orbit suggesting it has made at least one passage through the Milky Way disk. A magnetic field found around this cloud has been thought to provide extra stability as it passes through the Galactic halo. We use the Karl G. Jansky Very Large Array to measure Faraday rotation measures (RMs) toward 1105 extragalactic background point sources behind and next to the Smith Cloud to constrain the detailed geometry and strength of its magnetic field. The RM pattern across the cloud gives the detailed morphology of the magnetic field structure, which indicates a field draped over the ionized gas and compressed at the head of the cloud. We constrain the peak line-of-sight magnetic field strength to ≿+5 μG and create a model of the magnetic field to demonstrate that a draped configuration can qualitatively explain the morphology of the observed RMs. ; Peer reviewed: Yes ; NRC publication: Yes
نوع الوثيقة: article in journal/newspaper
وصف الملف: text
اللغة: English
تدمد: 1538-4357
Relation: The Astrophysical Journal, Volume: 871, Issue: 2, Publication date: 2019-02-01
DOI: 10.3847/1538-4357/aaf886
الاتاحة: https://doi.org/10.3847/1538-4357/aaf886
https://nrc-publications.canada.ca/eng/view/object/?id=f72340df-b0b2-4828-9374-a0cfaf98a7ec
https://nrc-publications.canada.ca/fra/voir/objet/?id=f72340df-b0b2-4828-9374-a0cfaf98a7ec
رقم الانضمام: edsbas.43DB8C1C
قاعدة البيانات: BASE
الوصف
تدمد:15384357
DOI:10.3847/1538-4357/aaf886