Diffuse Interstellar Bands in the Young Galactic Clusters M16 and M17

Pfau, W.; Henning, Th.

doi:10.1007/978-94-011-0373-2_12

W. Pfau³ &
Th. Henning⁴

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 202))

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Abstract

The closely related galactic clusters M16 and M17 were selected for spectroscopy around the DIBs λλ5780/5797 and λ6203 for the anomalous reddening law prevailing therein. It is evident that the band strengths differ markedly between and that there is no increase of DIB strength within the clusters.

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Authors and Affiliations

University Observatory, Jena, Germany
W. Pfau
Research Group of the Max Planck Society, Jena, Germany
Th. Henning

Authors

W. Pfau
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Th. Henning
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Editor information

Editors and Affiliations

NASA Ames Research Center, Moffett Field, CA, USA
A. G. G. M. Tielens
Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO, USA
T. P. Snow

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Pfau, W., Henning, T. (1995). Diffuse Interstellar Bands in the Young Galactic Clusters M16 and M17. In: Tielens, A.G.G.M., Snow, T.P. (eds) The Diffuse Interstellar Bands. Astrophysics and Space Science Library, vol 202. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0373-2_12

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DOI: https://doi.org/10.1007/978-94-011-0373-2_12
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4167-6
Online ISBN: 978-94-011-0373-2
eBook Packages: Springer Book Archive

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