ISO impact on stellar models and vice versa

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dc.creatorDecin, L.
dc.creatorWaelkens, C.
dc.creatorEriksson, K.
dc.creatorGustafsson, B.
dc.creatorPlez, B.
dc.creatorSauval, A. J.
dc.creatorVan Assche, W.
dc.creatorVandenbussche, B.
dc.date2000-08-23
dc.date.accessioned2026-07-07T01:55:04Z
dc.date.available2026-07-07T01:55:04Z
dc.descriptionWe present a detailed spectroscopic study of a sample of bright, mostly cool, stars observed with the Short-Wavelength Spectrometer (SWS) on board the Infrared Space Observatory (ISO), which enables the accurate determination of the stellar parameters of the cool giants, but also serves as a critical review of the ISO-SWS calibration.
dc.description6 pages, 3 figures, to appear in `ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy', held 2-4 February 2000, at VILSPA
dc.identifierhttps://arxiv.org/abs/astro-ph/0008362
dc.identifierhttp://arxiv.org/abs/astro-ph/0008362
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1530
dc.subjectAstrophysics
dc.titleISO impact on stellar models and vice versa
dc.typetext

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