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Supergiant Stars as Abundance Probes

  • L. R. Patrick (a1) (a2), C. J. Evans (a3), B. Davies (a4) and R.-P. Kudritzki (a5) (a6)

Abstract

By compiling abundances from red and blue supergiants (SGs) within the Local Universe, I present the Mass-Metallicity relation (MZR) using stellar tracers, demonstrating the excellent internal consistency. Comparing this result with nebular tracers, those empirically calibrated to direct-method studies provide the most consistent results.

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Andrews, B. H., & Martini, P. 2013, ApJ, 765, 14010.1088/0004-637X/765/2/140
Davies, B., Kudritzki, R.-P., Lardo, C., et al. 2017, ApJ, 847, 11210.3847/1538-4357/aa89ed
Evans, C. J., Davies, B., Kudritzki, R.-P., et al. 2011, A&A, 527, A50
Gazak, J. Z., Kudritzki, R., Evans, C., et al. 2015, ApJ, 805, 18210.1088/0004-637X/805/2/182
Patrick, L. R., Evans, C. J., Davies, B., et al. 2017, MNRAS, 468, 49210.1093/mnras/stx410
Tremonti, C. A., Heckman, T. M., Kauffmann, G., et al. 2004, ApJ, 613, 89810.1086/423264
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Supergiant Stars as Abundance Probes

  • L. R. Patrick (a1) (a2), C. J. Evans (a3), B. Davies (a4) and R.-P. Kudritzki (a5) (a6)

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