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Morpho-Kinematics of the Circumstellar Environments around Post-AGB Stars

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 نشر من قبل Toshiya Ueta
 تاريخ النشر 2018
  مجال البحث فيزياء
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We observed two proto-planetary nebulae, HD 56126 representing a source with an elliptical circumstellar shell and IRAS 16594-4656 representing a source with a bipolar circumstellar shell, with ALMA in the 12CO and 13CO J=3-2 lines and neighboring continuum to see how the morpho-kinematics of CO gas and dust emission properties in their circumstellar environments differ.



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