Hostname: page-component-784d4fb959-mvngg Total loading time: 0 Render date: 2025-07-16T11:19:16.434Z Has data issue: false hasContentIssue false

The Effect Of Alpha-Element Enhancement On Surface Brightness Fluctuation Magnitudes And Broad-Band Colors

Published online by Cambridge University Press:  01 December 2006

Hyun-chul Lee
Affiliation:
Washington State University email: hclee@wsu.edu
Guy Worthey
Affiliation:
Washington State University email: hclee@wsu.edu
John P. Blakeslee
Affiliation:
Washington State University email: hclee@wsu.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present the effects due to alpha-element enhancement on surface brightness fluctuation magnitudes and broad-band colors in order to investigate the calibration zero-point. We study these effects at ages covering 0.1 to 13 Gyr and metallicities of Z=0.0003 to 0.04 using the Teramo group's isochrones, BaSTI. Our preliminary results indicate that alpha-enhanced models are needed to match massive red galaxies while solar-scaled models are fine for dwarf blue galaxies to reproduce their independently estimated ages and metallicities.

References

Blakeslee, J.P., Lucey, J.R., Tonry, J.L. et al. 2002, MNRAS, 330, 443CrossRefGoogle Scholar
Cordier, D., Pietrinferni, A., Cassisi, S., & Salaris, M. 2007, AJ, 133, 468CrossRefGoogle Scholar
Mei, s., Blakeslee, J.P., Tonry, J.L. et al. 2005, ApJ, 625, 121CrossRefGoogle Scholar
Mieske, S., Hilker, M., & Infante, L. 2006, A&A, 458, 1013Google Scholar
Pietrinferni, A., Cassisi, S., Salaris, M., & Castelli, F. 2004, ApJ, 612, 168CrossRefGoogle Scholar
Pietrinferni, A., Cassisi, S., Salaris, M., & Castelli, F. 2006, ApJ, 642, 797CrossRefGoogle Scholar