Polarization as a Probe of Thick Dust Disks in Edge-on Galaxies: Application to NGC 891
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/862/i=1/a=87/pdf
Reference47 articles.
1. EFFICIENT THREE-DIMENSIONAL NLTE DUST RADIATIVE TRANSFER WITH SKIRT
2. Monte Carlo Simulations of Dusty Spiral Galaxies: Extinction and Polarization Properties
3. Halo dust detection around NGC 891
4. Mid‐Infrared Photometry of Dust in the Thick Disk of NGC 891
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1. Exploring the Magnetic Field Geometry in NGC 891 with SOFIA/HAWC+;The Astronomical Journal;2023-05-03
2. Paradigmatic examples for testing models of optical light polarization by spheroidal dust;Astronomy & Astrophysics;2023-05
3. The distribution of dust in edge-on galaxies: I. The global structure;Monthly Notices of the Royal Astronomical Society;2022-07-31
4. Lyα Radiative Transfer: A Stokes Vector Approach to Lyα Polarization;The Astrophysical Journal Supplement Series;2022-02-17
5. HAWC+ Far-infrared Observations of the Magnetic Field Geometry in M51 and NGC 891;The Astronomical Journal;2020-09-21
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