POLARIZATION MEASUREMENTS OF HOT DUST STARS AND THE LOCAL INTERSTELLAR MEDIUM

POLARIZATION MEASUREMENTS OF HOT DUST STARS AND THE LOCAL INTERSTELLAR MEDIUM

Debris discs are typically revealed through the presence of excess emission at infrared wavelengths. Most discs exhibit excess at mid- and far-infrared wavelengths, analogous to the solar system's Asteroid and Edgeworth-Kuiper belts. Recently, stars with strong (similar to 1%) excess at near-in...

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Bibliographic Details
Main Authors: Marshall, J. P., Cotton, D. V., Bott, K., Ertel, S., Kennedy, G. M., Wyatt, M. C., Burgo, C. del, Absil, O., Bailey, J., Kedziora-Chudczer, L.
Other Authors: Univ Arizona, Dept Astron, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
circumstellar matter
dust
extinction
planetary systems
polarization
Online Access:http://hdl.handle.net/10150/621381
http://arizona.openrepository.com/arizona/handle/10150/621381

Internet

http://hdl.handle.net/10150/621381
http://arizona.openrepository.com/arizona/handle/10150/621381

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