Grain size constraints on HL Tau with polarization signature
The millimeter-wave polarization of the protoplanetary disk around HL Tau has been interpreted as the emission from elongated dust grains aligned with the magnetic field in the disk. However, the self-scattering of thermal dust emission may also explain the observed millimeter-wave polarization. In...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
2015
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1507.08902
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| Author Notes: | Akimasa Kataoka, Takayuki Muto, Munetake Momose, Takashi Tsukagoshi, Cornelis P. Dullemond |
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