Millimeter-wave polarization of protoplanetary disks due to dust scattering
We present a new method to constrain the grain size in protoplanetary disks with polarization observations at millimeter wavelengths. If dust grains are grown to the size comparable to the wavelengths, the dust grains are expected to have a large scattering opacity and thus the continuum emission is...
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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/1504.04812
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| Author Notes: | Akimasa Kataoka, Takayuki Muto, Munetake Momose, Takashi Tsukagoshi, Misato Fukagawa, Hiroshi Shibai, Tomoyuki Hanawa, Koji Murakawa, Cornelis P. Dullemond |
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