The chemistry of Interstellar Dust through the X-ray Absorption fine Structures (XAFS) in GX 9+1

Details The chemistry of Interstellar Dust through the X-ray Absorption fine Structures (XAFS) in GX 9+1 The chemistry of Interstellar Dust through the X-ray Absorption fine Structures (XAFS) in GX 9+1

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1918m&link_type=abstract

Chandra Proposal ID #07400039

Computer Science

Chandra Proposal Id #07400039

Scientific paper

We propose to observe the bright X-ray compact source GX 9+1 with the
HETGS-ACIS-S of Chandra. The spectrum displays complex features in the
vicinity of the Mg and Si absorption edges. These features are believed
to be produced by absorption from interstellar dust grains (X-ray
Absorption Fine Structure, XAFS), possibly in the form of silicates.

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