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Detectability of Wolf-Rayet stars in M33 and Beyond the Local Group

Published online by Cambridge University Press:  28 July 2017

Aaron J. Brocklebank ,
J. L. Pledger  and
A. E. Sansom
Aaron J. Brocklebank
Affiliation:
Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK email: ajbrocklebank1@uclan.ac.uk
J. L. Pledger
Affiliation:
Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK email: ajbrocklebank1@uclan.ac.uk
A. E. Sansom
Affiliation:
Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK email: ajbrocklebank1@uclan.ac.uk
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Abstract

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To understand how complete our surveys of Wolf-Rayet (WR) stars can be with the current generation of telescopes, we study images of M33, a galaxy with a nearly complete WR catalogue, and degrade them to investigate the detectability of WRs out to 30Mpc. We lose almost half of our sample at 4.2Mpc, and at 30Mpc we detect only those WRs in bright regions.

Keywords

stars: Wolf-Rayetstars: statisticsgalaxies: stellar contentgalaxies: individual: M33
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 388
Copyright
Copyright © International Astronomical Union 2017 

References

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