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What can the UV SED tell us about primitive galaxies?

Published online by Cambridge University Press:  17 August 2012

Sara R. Heap
Sara R. Heap*
Affiliation:
NASA's Goddard Space Flight Center, Code 667, Greenbelt Maryland, U.S.A. email: Sally.Heap@NASA.gov
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Abstract

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We use the full SED of a well observed dwarf galaxy, I Zw 18, to evaluate what inferences can be made about very high-redshift galaxies from their UV SED's alone.

Keywords

galaxies: evolutiondwarfindividual (I Zw 18)high-redshiftstellar content
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S284: The Spectral Energy Distribution of Galaxies , September 2011 , pp. 49 - 52
Copyright
Copyright © International Astronomical Union 2012

References

Aloisi, A., Clementini, G., Tosi, M., et al. 2007, ApJ, 667, L151.CrossRefGoogle Scholar
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., et al. 2010, ApJ (Letters), 708, L69.CrossRefGoogle Scholar
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., et al. 2011, astro-ph 1109.0994v1Google Scholar
Calzetti, D., Kinney, A., & Storchi-Bergmann, T. 1994, ApJ, 429, 582CrossRefGoogle Scholar
Castelli, F. & Kurucz, R. 2004, wwwuser.oat.ts.astro.it/castelli/grids.htmlGoogle Scholar
Contreras Ramos, R., Annibali, F., Fiorentino, G., Tosi, M., et al. 2011, astro-ph 1106.5613v1Google Scholar
Dufour, R. & Hester, J. 1990, ApJ, 350, 149CrossRefGoogle Scholar
Ferland, G., Korista, K., Verner, D., et al. 1998, PASP, 110, 761CrossRefGoogle Scholar
Finkelstein, S., Papovich, S., Giavalisco, M. et al. 2010, ApJ, 719, 1250CrossRefGoogle Scholar
Herrara-Camus, R., Bolatto, A., Leroy, A. et al. 2010, www.astro.umd.edu/~rhc/Herrera_IZw18.pdfGoogle Scholar
Lejeune, T. & Schaerer, D. 2001, A&A, 366, 538Google Scholar
Meurer, G., Heckman, T., & Calzetti, D. 1999, ApJ, 521, 64CrossRefGoogle Scholar
Reines, A., Nidever, D., Whelan, D., & Johnson, K. 2010, ApJ, 708, 26CrossRefGoogle Scholar
Schaerer, D. 2002, A&A, 382, 28Google Scholar
Thuan, T. 2008, in: Hunt, L., Madden, S. & Schneider, R. (eds.), Low-Metalllicity Star Formation, IAU Symp. 255, (CUP), p. 348Google Scholar
van Zee, L., Westpfahl, D., Haynes, M., & Salzer, J. 1998, AJ, 115, 1000CrossRefGoogle Scholar
van Zee, L., Cannon, J., & Skillman, E. 2006, BAAS, Vol. 38, p. 1136Google Scholar