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The grey extinction curve in NGC 3603

Published online by Cambridge University Press:  07 March 2016

Xiaoying Pang ,
Anna Pasquali  and
Eva K. Grebel
Xiaoying Pang
Affiliation:
Shanghai Institute of Technology, 100 Haiquan Road, Fengxian district, Shanghai 201418, China email: [email protected]
Anna Pasquali
Affiliation:
Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12–14, 69120 Heidelberg, Germany
Eva K. Grebel
Affiliation:
Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12–14, 69120 Heidelberg, Germany
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Abstract

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We use photometry in the F220W, F250W, F330W, F435W filters from the High Resolution Channel of the Advanced Camera for Surveys and photometry in the F555W, F675W, and F814W filters from the Wide Field and Planetary Camera 2 aboard the Hubble Space Telescope to derive individual stellar reddenings and extinctions for member stars in the HD 97950 cluster in the giant H ii region NGC 3603. Within the standard deviation associated with E(λ−F555W)/E(F435W−F555W) in each filter, the cluster extinction curve at ultraviolet wavelengths tends to be greyer than the average Galactic extinction laws from Cardelli et al. (1989) and Fitzpatrick et al. (1999). It is closer to the extinction law derived by Calzetti et al. (2000) for starburst galaxies, where the 0.2175 μm bump is absent.

Keywords

star clusterextinctionreddening
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S312: Star Clusters and Black Holes in Galaxies across Cosmic Time , August 2014 , pp. 243 - 244
Copyright
Copyright © International Astronomical Union 2016 

References

Calzetti, D., Armus, L., Bohlin, R. C., et al. 2000, ApJ, 533, 682CrossRefGoogle Scholar
Cardelli, J. A., Clayton, G. C., & Mathis, J. S. 1989, ApJ, 345, 245CrossRefGoogle Scholar
Fitzpatrick, E. L. 1999, PASP, 111, 63CrossRefGoogle Scholar
Pandey, A. K., Ogura, K., & Sekiguchi, K. 2000, PASJ, 52, 847CrossRefGoogle Scholar
Pang, X., Grebel, E. K., Allison, R. J., et al. 2013, ApJ, 764, 73CrossRefGoogle Scholar