Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-24T02:01:11.423Z Has data issue: false hasContentIssue false
  • English
  • Français

What can the Occult do for you? STarlight Attenuation & Reddening Survey of Multiple Occulting Galaxies (STARSMOG)

Published online by Cambridge University Press:  27 October 2016

B. W. Holwerda  and
W. C. Keel
B. W. Holwerda
Affiliation:
Leiden Observatory email: [email protected] twitter: @benneholwerda
W. C. Keel
Affiliation:
Alabama email: [email protected] twitter: @NGC3314
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.

Interstellar dust is still the 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 HST observation of occulting galaxy pairs to accurately map the distribution of dust in foreground galaxies in fine (<100 pc) detail. Furthermore, Integral Field Unit observations of such pairs will map the effective extinction curve in these occulting galaxies, 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: the dust geometry, a probability function of the amount of dimming as a function of galaxy type, its dependence on wavelength, and evolution of all these properties with cosmic time using distant, high-redshift pairs.

Keywords

Keyword1keyword2keyword3etc
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 173 - 175
Copyright
Copyright © International Astronomical Union 2016 

References

Albrecht, A. et al. 2006, astro-ph/0609591Google Scholar
Allaert, F. et al. 2015, ArXiv e-printsGoogle Scholar
Holwerda, B. W. 2008, MNRAS, 386, 475 Google Scholar
Holwerda, B. W. et al. 2015a, MNRAS, 449, 4277 CrossRefGoogle Scholar
Holwerda, B. W. et al. 2012, A&A, 541, L5 Google Scholar
Holwerda, B. W. et al. 2013, MNRAS, 433, 47 Google Scholar
Holwerda, B. W. & Keel, W. C. 2013, A&A, 556, A42 Google Scholar
Holwerda, B. W. et al. 2007, AJ, 134, 2385 Google Scholar
Holwerda, B. W. et al. 2015b, MNRAS, 451, 2390 Google Scholar
Holwerda, B. W. et al. 2009, AJ, 137, 3000 Google Scholar
Holwerda, B. W. et al. 2015c, MNRAS, 446, 3768 Google Scholar
Keel, W. C. et al. 2014, AJ, 147, 44 Google Scholar
Keel, W. C. et al. 2013, PASP, 125, 2 Google Scholar
Riess, A. G. et al. 2011, ApJ, 730, 119 Google Scholar
Robotham, A. S. G. et al. 2014, MNRAS, 444, 3986 Google Scholar
Verstappen, J. et al. 2013, A&A, 556, A54 Google Scholar