Probing Sub-parsec Structure in the Lyman Alpha Forest with Gravitational Microlensing

Abstract

We present the results of microlens ray-tracing simulations showing the effect of absorbing material between a source quasar and a lensing galaxy in a gravitational lens system. We find that, in addition to brightness fluctuations due to microlensing, the strength of the absorption line relative to the continuum varies with time, with the properties of the variations depending on the structure of the absorbing material. We conclude that such variations will be measurable via UV spectroscopy of image A of the gravitationally lensed quasar Q2237+0305 if the Lyman Alpha clouds between the quasar and the lensing galaxy possess structure on scales smaller than $\sim 0.1$ pc. The time scale for the variations is on the order of order years to decades, although very short term variability can occur. While the Lyman alpha lines may not be accessible at all wavelengths, this approach is applicable to any absorption system, including metal lines.

8 pages, 11 figures, to appear in MNRAS (note resolution of some figures reduced due to size limitations)

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Cited by in corpus (2)

• Probing ~100 AU Intergalactic MgII Absorbing "Cloudlets" with Quasar Microlensing
• Gravitational Microlensing as a probe of the Electron Scattering Region in Q2237+0305