Toward a Removal of Temperature Dependencies from Abundance Determinations: NGC 628
Abstract
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.
Additional Information
© 2013 American Astronomical Society. Received 2013 August 1; accepted 2013 September 2; published 2013 October 18. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. We thank the referee for a quick and thoughtful report that has improved this paper. K.V.C. thanks Rick Pogge and Brett Andrews for enlightening discussions on this topic. PACS has been developed by a consortium of institutes led by MPE (Germany) and including UVIE (Austria); KU Leuven, CSL, IMEC (Belgium); CEA, LAM (France); MPIA (Germany); INAF-IFSI/OAA/OAP/OAT, LENS, SISSA (Italy); IAC (Spain). This development has been supported by the funding agencies BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI/INAF (Italy), and CICYT/MCYT (Spain). HIPE is a joint development by the Herschel Science Ground Segment Consortium, consisting of ESA, the NASA Herschel Science Center, and the HIFI, PACS and SPIRE consortia. This work is based (in part) on observations made with Herschel, a European Space Agency Cornerstone Mission with significant participation by NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.Attached Files
Published - 0004-637X_777_2_96.pdf
Submitted - 1309.0817v1.pdf
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Additional details
- Alternative title
- Towards A Removal of Temperature Dependencies from Abundance Determinations
- Eprint ID
- 42773
- Resolver ID
- CaltechAUTHORS:20131202-114919984
- Bundesministerium für Verkehr, Innovation und Technologie (BMVIT)
- ESA-PRODEX (Belgium)
- Commissariat à l'Energie Atomique (CEA)
- Deutschen Zentrums für Luft- und Raumfahrt (DLR)
- Agenzia Spaziale Italiana (ASI)
- CICYT/MCYT (Spain)
- NASA/JPL/Caltech
- Centre National d'Études Spatiales (CNES)
- Istituto Nazionale di Astrofisica (INAF)
- Created
-
2013-12-02Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)