Could the shape of Mrk 205 Fe Kα line be explaned by microlensing effect?

Details Could the shape of Mrk 205 Fe Kα line be explaned by microlensing effect? Could the shape of Mrk 205 Fe Kα line be explaned by microlensing effect?

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pobeo..73..215p&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 73, p. 215 - 218 (2002). In: Proceedings of the T

Astronomy and Astrophysics

Astronomy

1

Active Galactic Nuclei, Spectral Lines, Microlensing

Scientific paper

We discuss the unusual shape of Mrk 205 Fe Kα line in the light of microlensing influence of a caustic from the galaxy NGC 4319. The shape of the Fe Kα line may be described as disc emitted line deformed by microlensing effect of a star with mass less than 0.2 Msolar from the NGC 4319 star disc. In the paper we discuss the two scenarious of line variation, if the microlensing effect is present.

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