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The Search for Wolf-Rayet Stars in IC10

Published online by Cambridge University Press:  28 July 2017

Katie Tehrani
Affiliation:
Department of Physics & Astronomy, University of Sheffield, Hounsfield Road, S3 7RH, Sheffield, UK email: k.tehrani@sheffield.ac.uk
Paul Crowther
Affiliation:
Department of Physics & Astronomy, University of Sheffield, Hounsfield Road, S3 7RH, Sheffield, UK email: k.tehrani@sheffield.ac.uk
Isabelle Archer
Affiliation:
Department of Physics & Astronomy, University of Sheffield, Hounsfield Road, S3 7RH, Sheffield, UK email: k.tehrani@sheffield.ac.uk
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Abstract

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We present a deep imaging and spectroscopic survey of the Local Group starburst galaxy IC10 using Gemini North/GMOS to unveil the global Wolf-Rayet population. It has previously been suggested that for IC10 to follow the WC/WN versus metallicity dependence seen in other Local Group galaxies, a large WN population must remain undiscovered. Our search revealed 3 new WN stars, and 5 candidates awaiting confirmation, providing little evidence to support this claim. We also compute an updated nebular derived metallicity of log(O/H)+12=8.40 ± 0.04 for the galaxy using the direct method. Inspection of IC10 WR average line luminosities show these stars are more similar to their LMC, rather than SMC counterparts.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

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