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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 693803.0, MPI für Astronomie / Publikationen_mpia
Toward a removal of temperature dependencies from abundance determinations: NGC 628
Authors:Croxall, K. V.; Smith, J. D.; Brandl, B. R.; Groves, B. A.; Kennicutt, R. C.; Kreckel, K.; Johnson, B. D.; Pellegrini, E.; Sandstrom, K. M.; Walter, F.; Armus, L.; Beirão, P.; Calzetti, D.; Dale, D. A.; Galametz, M.; Hinz, J. L.; Hunt, L. K.; Koda, J.; Schinnerer, E.
Date of Publication (YYYY-MM-DD):2013
Title of Journal:The Astrophysical Journal
Volume:777
Start Page:id. 96 (9 pp)
Audience:Not Specified
Abstract / Description:The metal content of a galaxy, a key property for distinguishing between viable galaxy evolutionary scenarios, strongly influences many of the physical processes in the interstellar medium. An absolute and robust determination of extragalactic metallicities is essential in constraining models of chemical enrichment and chemical evolution. Current gas-phase abundance determinations, however, from optical fine-structure lines are uncertain to 0.8 dex as conversion of these optical line fluxes to abundances is strongly dependent on the electron temperature of the ionized gas. In contrast, the far-infrared (far-IR) emission lines can be used to derive an O++ abundance that is relatively insensitive to temperature, while the ratio of the optical to far-IR lines provides a consistent temperature to be used in the derivation of an O+ abundance. We present observations of the [O III] 88 μm fine-structure line in NGC 628 that were obtained as part of the Key Insights on Nearby Galaxies: a Far Infared Survey with Herschel program. These data are combined with optical integrated field unit data to derive oxygen abundances for seven H II regions. We find the abundance of these regions to all lie between the high and low values of strong-line calibrations and to be in agreement with estimates that assume temperature fluctuations are present in the H II regions. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.
Free Keywords:galaxies: abundances; galaxies: individual: NGC 628; galaxies: ISM; H II regions; infrared: ISM; ISM: abundances
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0004-637X %R 10.1088/0004-637X/777/2/96
URL:http://cdsads.u-strasbg.fr/abs/2013ApJ...777...96C
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