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SFR and Abundances of Nearby Galaxies

Part of: IAU Issue 315 - From Interstellar Clouds...

Published online by Cambridge University Press:  12 September 2016

Marianne Takamiya ,
Daniel Berke ,
Forrest Bremer ,
Casey Jones  and
Guillaume Poquet
Marianne Takamiya
Affiliation:
Department of Physics and Astronomy, University of Hawai'i Hilo, 200 Kawili Street, Hilo, HI 96720, USA email: [email protected]
Daniel Berke
Affiliation:
EOA, 660 N. A'ohoku Place, Hilo, HI 96720, USA
Forrest Bremer
Affiliation:
Department of Physics and Astronomy, University of Hawai'i Hilo, 200 Kawili Street, Hilo, HI 96720, USA email: [email protected]
Casey Jones
Affiliation:
Department of Physics and Astronomy, University of Hawai'i Hilo, 200 Kawili Street, Hilo, HI 96720, USA email: [email protected]
Guillaume Poquet
Affiliation:
ESTACA, Campus-Ouest, Rue Georges Charpak, BP 76121 Box 53061 Laval Cedex 9, France
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Abstract

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We present star formation rates and nebular abundances of 59 different star-forming regions in 16 nearby galaxies. The star-forming regions were selected to be bright in Hα and were observed with the SNIFS integral field spectrograph on the UH 2.2m telescope. The spectra span the wavelength range between 3200Å and 1μm. We find that the local star formation rates depend on the local abundances in that low SFRs show a dependence but high SFR appear insensitive to it.

Keywords

galaxies: abundancesgalaxies: ISM
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S315: From Interstellar Clouds to Star-Forming Galaxies: Universal Processes? , August 2015 , E73
Copyright
Copyright © International Astronomical Union 2016 

References

Aldering, G. et al. 2002, in Proc. SPIE, ed. Tyson, J. A. & Wolff, S., Vol. 4836, p1Google Scholar
Pettini, M & Pagel, B. E. J. 2004, MNRAS, 348, 59L Google Scholar