How to search for AGB stars in the near-IR post-starburst spectra

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dc.creatorLancon, A.
dc.creatorMouhcine, M.
dc.creatorFioc, M.
dc.creatorSilva, D.
dc.date1999-03-09
dc.date.accessioned2026-07-07T02:30:45Z
dc.date.available2026-07-07T02:30:45Z
dc.descriptionBased on evolutionary spectral synthesis models explicitly including the spectra of variable AGB stars, we select near-IR features that dentify the strong O-rich or C-rich AGB contributions to the near-IR light of post-starburst populations. AGB temperature scales and lifetimes remain major sources of uncertainties. We discuss applications and suggest massive post-starburst clusters as prime targets for observational tests.
dc.description4 pages, 3figures, accepted for publication in A&A Letters
dc.identifierhttps://arxiv.org/abs/astro-ph/9903135
dc.identifierhttp://arxiv.org/abs/astro-ph/9903135
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13922
dc.subjectAstrophysics
dc.titleHow to search for AGB stars in the near-IR post-starburst spectra
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