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What can the occult do for you?

Published online by Cambridge University Press:  21 March 2017

B. W. Holwerda  and
W. C. Keel
B. W. Holwerda
Affiliation:
Sterrenwacht, University of Leiden, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands email: [email protected] twitter: @benneholwerda
W. C. Keel
Affiliation:
Dept. of Physics & Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487, USA email: [email protected] twitter: @NGC3314
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Abstract

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Interstellar dust is still a dominant uncertainty in Astronomy, limiting precision in e.g., cosmological distance estimates and models of how light is re-processed within a galaxy. When a foreground galaxy serendipitously overlaps a more distant one, the latter backlights the dusty structures in the nearer foreground galaxy.

Such an overlapping or occulting galaxy pair can be used to measure the distribution of dust in the closest galaxy with great accuracy. The STARSMOG program uses Hubble to map the distribution of dust in foreground galaxies in fine (<100 pc) detail. Integral Field Unit (IFU) observations will map the effective extinction curve, disentangling the role of fine-scale geometry and grain composition on the path of light through a galaxy.

The overlapping galaxy technique promises to deliver a clear understanding of the dust in galaxies: geometry, a probability function of dimming as a function of galaxy mass and radius, and its dependence on wavelength.

Keywords

ISM: dustextinction ISM: structuregalaxies: dwarfgalaxies: ISMgalaxies: spiralgalaxies: structure (cosmology:) distance scaleultraviolet: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S321: Formation and Evolution of Galaxy Outskirts , March 2016 , pp. 248 - 250
Copyright
Copyright © International Astronomical Union 2017 

References

Calzetti, D. & Heckman, T. M. 1999, ApJ, 519, 27 CrossRefGoogle Scholar
Calzetti, D. et al. 1994, ApJ, 429, 582 CrossRefGoogle Scholar
Cardelli, J. A. et al. 1989, ApJ, 345, 245 CrossRefGoogle Scholar
Charlot, S. & Fall, S. M. 2000, ApJ, 539, 718 CrossRefGoogle Scholar
Domingue, D. L. et al. 2000, ApJ, 545, 171 CrossRefGoogle Scholar
Holwerda, B. W. et al. 2015, MNRAS 449 4277–4287 CrossRefGoogle Scholar
Holwerda, B. W. et al. 2013, MNRAS, 433, 47 CrossRefGoogle Scholar
Holwerda, B. W. & Keel, W. C. 2013, A&A, 556, A42 Google Scholar
Holwerda, B. W. et al. 2007, AJ, 134, 2385 CrossRefGoogle Scholar
Holwerda, B. W. et al. 2009, AJ, 137, 3000 CrossRefGoogle Scholar
Holwerda, B. W. et al. 2014, ApJ, 788, 77 CrossRefGoogle Scholar
Keel, W. C. et al. 2014, AJ, 147, 44 CrossRefGoogle Scholar
Keel, W. C. et al. 2013, PASP, 125, 2 CrossRefGoogle Scholar
Keel, W. C., & White, R. E. III 2001a, AJ, 121, 1442 CrossRefGoogle Scholar
Keel, W. C., & White, R. E. III 2001b, AJ, 122, 1369 CrossRefGoogle Scholar
White, R. E. III et al. 2000, ApJ, 542, 761 CrossRefGoogle Scholar
Wild, V. et al. 2011, MNRAS, 417, 1760 CrossRefGoogle Scholar