X-ray absorption and rapid variability of the dwarf Seyfert nucleus of NGC4395

Details X-ray absorption and rapid variability of the dwarf Seyfert nucleus of NGC4395 X-ray absorption and rapid variability of the dwarf Seyfert nucleus of NGC4395

2000-06-29

arxiv.org/abs/astro-ph/0006427v1

Mon.Not.Roy.Astron.Soc.318:879,2000

Astronomy and Astrophysics

Astrophysics

12 pages, accepted for publication in MNRAS

Scientific paper

10.1046/j.1365-8711.2000.03810.x

We report the detection of an absorbed central X-ray source and its strong, rapid variability in NGC4395, the least luminous Seyfert nucleus known. The X-ray source exhibits a number of flares with factors of 3-4 flux changes during a half day ASCA observation. Such X-ray variability is in constrast to the behaviour of other low luminosity active galaxies. It provides further support for an accreting black hole model rather than an extreme stellar process in accounting for the nuclear activity of NGC4395. The soft X-ray emission below 3 keV is strongly attenuated by absorption. The energy spectrum in this absorption band shows a dramatic change in response to the variation in continuum luminosity. A variable warm absorber appears to be an explanation for the spectral change. The absorption-corrected 2-10 keV luminosity is 4e39 erg/s for a source distance of 2.6 Mpc, and at 1 keV is one order of magnitude above previous ROSAT estimates. Our X-ray results infer the nuclear source of NGC4395 to be a scaled-down version of higher luminosity Seyfert nuclei, with an intermediate mass (10^4-10^5 Msun) black hole, unlike the nearby low luminosity active galaxies in which underfed massive black holes are suspected to reside.

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