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Edge-on Low Surface Brightness Galaxies in the SDSS and the Red Halo Phenomenon

Published online by Cambridge University Press:  01 August 2006

Brady Caldwell
Affiliation:
Department of Astronomy and Space Physics, Uppsala University, Sweden email: brady.caldwell@astro.uu.se, nils.bergvall@astro.uu.se
Nils Bergvall
Affiliation:
Department of Astronomy and Space Physics, Uppsala University, Sweden email: brady.caldwell@astro.uu.se, nils.bergvall@astro.uu.se
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Abstract

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Extremely red halos have been detected around high surface brightness (HSB) disk galaxies and blue compact galaxies. We analyse the halo emission of a sample of 970 stacked edge-on low surface brightness (LSB) galaxies in the SDSS (DR4) down to μg ~ 30 mag arcsec−2. These are divided by gr colour limits into a “blue” Sample A (336 galaxies), “yellow” Sample B (318 galaxies) and “red” Sample C (316 galaxies). The gri colours indicate a prominent red excess in the polar direction, strongly deviating from any normal stellar population.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Zackrisson, E. 2006, ApJ 650, 812.CrossRefGoogle Scholar
Zibetti, S. 2004, MNRAS 347, 556.CrossRefGoogle Scholar