Temperature predictions for dust embedded AGB stars: how far can we go with synthetic near-infrared photometry ?

Simple item page
dc.creatorLastennet, E.
dc.creatorLorenz-Martins, S.
dc.creatorCuisinier, F.
dc.creatorLejeune, T.
dc.date2001-10-23
dc.date.accessioned2026-07-07T02:00:58Z
dc.date.available2026-07-07T02:00:58Z
dc.descriptionWe discuss the possibilities of the BaSeL models in its lowest temperature boundary (Teff ~ 2500 K for cool giants) to provide the Teff of AGB stars. We present the first step of our work, by comparing our predictions for the AGB star R Fornacis with the results of Lorenz-Martins & Lefevre (1994) based on the dust spectral energy distribution.
dc.descriptionTo appear in ASP Conference Series, proceedings of ``Observed HR diagrams and stellar evolution: the interplay between observational constraints and theory'' (Coimbra, Portugal, June 2001), eds., T. Lejeune & J. Fernandes
dc.identifierhttps://arxiv.org/abs/astro-ph/0110505
dc.identifierhttp://arxiv.org/abs/astro-ph/0110505
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3588
dc.subjectAstrophysics
dc.titleTemperature predictions for dust embedded AGB stars: how far can we go with synthetic near-infrared photometry ?
dc.typetext

Files

Collections

arXiv