Near Infrared Polarimetric Imaging of Giant HII Region RCW57
碩士 === 國立中央大學 === 天文研究所 === 96 === RCW57 is one of the brightest H II regions in the infrared harboring a group of massive stars with infrared excess indicative of their youth. We present the near-infrared JHKs polarization images taken by SIRPOL, an infrared polarimeter camera mounted on the IRSF (...
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ndltd-TW-096NCU051990032019-05-15T19:18:55Z http://ndltd.ncl.edu.tw/handle/kpytf6 Near Infrared Polarimetric Imaging of Giant HII Region RCW57 RCW57之近紅外偏極化影像觀測 Yi-Hsin Shih 施逸昕 碩士 國立中央大學 天文研究所 96 RCW57 is one of the brightest H II regions in the infrared harboring a group of massive stars with infrared excess indicative of their youth. We present the near-infrared JHKs polarization images taken by SIRPOL, an infrared polarimeter camera mounted on the IRSF (Infra-Red Survey Facility) telescope in Sutherland, South Africa. An overall scattering pattern is seen centrally symmetric around the luminous stellar group, indicating their dominant role in illuminating the nebulosity. Organized scattering patterns also reveal special dust distribution around embedded infrared sources, e.g., a dust ridge which may be associated with IRS−1 #60. We find no systematic polarization of background stars, which may indicate an entangled magnetic field structure in a turbulent environment of massive star formation. Wen-Ping Chen 陳文屏 學位論文 ; thesis 27 en_US |
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碩士 === 國立中央大學 === 天文研究所 === 96 === RCW57 is one of the brightest H II regions in the infrared harboring a group of massive stars with infrared excess indicative of their youth. We present the near-infrared JHKs polarization images taken by SIRPOL, an infrared polarimeter camera mounted on the IRSF (Infra-Red Survey Facility) telescope in Sutherland, South Africa. An overall scattering pattern is seen centrally symmetric around the luminous stellar group, indicating their dominant role in illuminating the nebulosity. Organized scattering patterns also reveal
special dust distribution around embedded infrared sources, e.g., a dust ridge which may be associated with IRS−1 #60. We find no systematic polarization of background stars, which may indicate an entangled magnetic field structure in a turbulent environment of massive star formation.
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author2 |
Wen-Ping Chen |
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Wen-Ping Chen Yi-Hsin Shih 施逸昕 |
author |
Yi-Hsin Shih 施逸昕 |
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Yi-Hsin Shih 施逸昕 Near Infrared Polarimetric Imaging of Giant HII Region RCW57 |
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Yi-Hsin Shih |
title |
Near Infrared Polarimetric Imaging of Giant HII Region RCW57 |
title_short |
Near Infrared Polarimetric Imaging of Giant HII Region RCW57 |
title_full |
Near Infrared Polarimetric Imaging of Giant HII Region RCW57 |
title_fullStr |
Near Infrared Polarimetric Imaging of Giant HII Region RCW57 |
title_full_unstemmed |
Near Infrared Polarimetric Imaging of Giant HII Region RCW57 |
title_sort |
near infrared polarimetric imaging of giant hii region rcw57 |
url |
http://ndltd.ncl.edu.tw/handle/kpytf6 |
work_keys_str_mv |
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