The Composition and Distribution of Dust Along the Line of Sight Towards the Galactic Center

Details The Composition and Distribution of Dust Along the Line of Sight Towards the Galactic Center The Composition and Distribution of Dust Along the Line of Sight Towards the Galactic Center

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456...45c&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Astronomy and Astrophysics

Astrophysics

2

Dust, Extinction, Ism: Molecules, Galaxy: Center, Infrared: Ism: Lines And Bands, Infrared: Stars

Scientific paper

We discuss the composition of dust and ice along the line of sight to the Galactic Center (GC) based on analysis of mid-infrared spectra (2.4-13 μm) from the Short Wavelength Spectrometer (SWS) on the Infrared Space Observatory (ISO). The complete results of this work appear in The Astrophysical Journal (Chiar et al. 2000; hereafter referred to as C00).

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