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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Main Authors: Yi-Hsin Shih, 施逸昕
Other Authors: Wen-Ping Chen
Format: Others
Language:en_US
Online Access:http://ndltd.ncl.edu.tw/handle/kpytf6
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spelling 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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description 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.
author2 Wen-Ping Chen
author_facet Wen-Ping Chen
Yi-Hsin Shih
施逸昕
author Yi-Hsin Shih
施逸昕
spellingShingle Yi-Hsin Shih
施逸昕
Near Infrared Polarimetric Imaging of Giant HII Region RCW57
author_sort 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
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