Post-AGB stars in the AKARI survey

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dc.creatorSiodmiak, Natasza
dc.creatorCox, Nick
dc.creatorSzczerba, Ryszard
dc.creatorGarcia-Lario, Pedro
dc.date2009-05-21
dc.date.accessioned2026-07-07T13:17:07Z
dc.date.available2026-07-07T13:17:07Z
dc.descriptionObscured 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.
dc.description4 pages, 5 figures, poster presented at the conference "AKARI, a light to illuminate the misty Universe", Tokyo, Japan, 16-19 February 2009
dc.identifierhttps://arxiv.org/abs/0905.3449
dc.identifierhttp://arxiv.org/abs/0905.3449
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/231011
dc.subjectSolar and Stellar Astrophysics
dc.titlePost-AGB stars in the AKARI survey
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