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Post-AGB stars in the AKARI survey

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 نشر من قبل Natasza Siodmiak
 تاريخ النشر 2009
  مجال البحث فيزياء
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Obscured by their circumstellar dusty envelopes post-AGB stars emit a large fraction of their energy in the infrared and thus, infrared sky surveys like IRAS were essential for discoveries of post-AGBs in the past. Now, with the AKARI infrared sky survey we can extend our knowledge about the late stages of stellar evolution. The long-term goal of our work is to define new photometric criteria to distinguish new post-AGB candidates from the AKARI data.



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