Simultaneous EUV and X-ray variability of NGC 4051
arXiv:astro-ph/9912103 · doi:10.1046/j.1365-8711.2000.03266.x
Abstract
We present a flux variability study of simultaneous RXTE and EUVE observations of the highly variable Seyfert galaxy NGC4051. We find a strong correlation between variability in the EUV and medium energy X-ray bands,indicating that both are sampling the same power-law continuum. The lag between the two bands is less than 20 ks and, depending on model assumptions, may be <1 ks. We examine the consequences of such a small lag in the context of simple Comptonisation models for the production of the power-law continuum. A lag of <1 ks implies that the size of the Comptonising region is less than 20 Schwarzschild radii for a black hole of mass >1E6 solar masses.
8 pages, accepted for publication in MNRAS
References in corpus (2)
Cited by in corpus (20)
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