The Structure and Variability of the Fe Kalpha line in NGC 3516

Details The Structure and Variability of the Fe Kalpha line in NGC 3516 The Structure and Variability of the Fe Kalpha line in NGC 3516

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprd11002t&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present new simultaneous XMM and Chandra HETG data from NGC 3516.
These data show a complex and variable profile for the Fe Kalpha line,
with significant changes occuring on timescales less than 1 day. These
results and their implications will be discussed in detail.

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