The 15-21 um PAH plateau

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dc.creatorPeeters, E.
dc.creatorMattioda, A. L.
dc.creatorKemper, F.
dc.creatorHudgins, D. M.
dc.creatorAllamandola, L. J.
dc.date2005-06-30
dc.date.accessioned2026-07-07T02:18:07Z
dc.date.available2026-07-07T02:18:07Z
dc.descriptionWe present 14--21 um emission spectra of star forming regions and compare them with the PAH spectra from the Ames PAH database. We show that while the emission in this region can be quite variable, the bulk of these variations can be accommodated by variations in the IS PAH population.
dc.descriptionconference proceedings of Spitzer New Views of the Cosmos, 2 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0507008
dc.identifierhttp://arxiv.org/abs/astro-ph/0507008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9372
dc.subjectAstrophysics
dc.titleThe 15-21 um PAH plateau
dc.typetext

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