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Polarization Mapping of Infrared Reflection Nebulae

Published online by Cambridge University Press:  04 August 2017

T. Nagata ,
T. Yamashita ,
S. Sato ,
M. Tanaka ,
S. Suzuki ,
N. Kaifu ,
I. McLean ,
J. Hough ,
I. Gatley  and
R. Garden
T. Nagata
Affiliation:
Dept. of Physics, Kyoto U., Kyoto 606, Japan
T. Yamashita
Affiliation:
Dept. of Physics, Kyoto U., Kyoto 606, Japan
S. Sato
Affiliation:
Dept. of Physics, Kyoto U., Kyoto 606, Japan
M. Tanaka
Affiliation:
Dept. of Physics, Kyoto U., Kyoto 606, Japan
S. Suzuki
Affiliation:
Nobeyama Radio Obs., U. of Tokyo, Nagano 384-13, Japan
N. Kaifu
Affiliation:
Nobeyama Radio Obs., U. of Tokyo, Nagano 384-13, Japan
I. McLean
Affiliation:
The Royal Obs. Edinburgh, Edinburgh EH9 3HJ, UK
J. Hough
Affiliation:
Hatfield Polytechnic Obs., Hertfordshire, SG13 8LD, UK
I. Gatley
Affiliation:
UKIRT, Hilo, Hawaii 96720, USA
R. Garden
Affiliation:
The Royal Obs. Edinburgh, Edinburgh EH9 3HJ, UK

Extract

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Extensive reflection nebulae have been discovered around GGD27 IRS and around W75N IRS by mapping the infrared polarization in the K band.

It was found that the infrared radiation from both objects is extended at λ = 2.2 μm, by using the Agematsu 1-m, the UH 2.2-m, and the UKIR 3.8-m telescopes. We have carried out polarization mapping with the Kyoto polarimeter on the UKIRT in August 1985.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 374 - 375
Copyright
Copyright © Reidel 1987