Summary
As part of the SINFONI science verification, we have performed AO supported integral field spectroscopy of the M17 silhouette disk. The results demonstrate that integral field spectroscopy at infrared wavelengths can add important pieces to the puzzle of high mass star formation.
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References
R. Chini, V. Hoffmeister, S. Kimeswenger et al: Nature 429, 155 (2004)
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D.E.A. Nürnberger, R. Chini, F. Eisenhauer et al: A&A submitted (2006)
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© 2007 Springer-Verlag Berlin Heidelberg
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Nürnberger, D.E.A. (2007). High Mass Star Formation In The Light Of Sinfoni. In: Kissler-Patig, M., Walsh, J.R., Roth, M.M. (eds) Science Perspectives for 3D Spectroscopy. Eso Astrophysics Symposia European Southern Observatory. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-73491-8_57
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DOI: https://doi.org/10.1007/978-3-540-73491-8_57
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-73490-1
Online ISBN: 978-3-540-73491-8
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