Physics
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..487m&link_type=abstract
Chandra Proposal ID #02600095
Physics
Chandra Proposal Id #02600095
Scientific paper
The presence of broad optical emission lines, indicating the presence of a LLAGN, in a significant subset of LINER galaxies has led to the expansion of the Seyfert 1/Seyfert 2 paradigm to LINER systems. However, the fraction of LINER 2 systems actually powered by LLAGN remains uncertain. This is an excellent problem for Chandra to address, since if a LLAGN (even a highly obscured example) is present then Chandra has the capabilities to identify it. We therefore propose an observation of the LINER 2 galaxy NGC 4111, a known X-ray source with a hitherto ambiguous central engine.
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