Volume 552, April 2013
|Number of page(s)||10|
|Section||Interstellar and circumstellar matter|
|Published online||04 April 2013|
Simulation of optical interstellar scintillation
Laboratoire de l’Accélérateur Linéaire, IN2P3 − CNRS, Université de
2 School of Astronomy, Institute for Research in Fundamental Sciences (IPM), PO Box 19395-5531, Tehran, Iran
3 Department of Physics, Sharif University of Technology, PO Box 11365-9161, Tehran, Iran
4 Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2L 2y5, Canada
Accepted: 6 February 2013
Aims. Stars twinkle because their light propagates through the atmosphere. The same phenomenon is expected on a longer time scale when the light of remote stars crosses an interstellar turbulent molecular cloud, but it has never been observed at optical wavelengths. The aim of the study described in this paper is to fully simulate the scintillation process, starting from the molecular cloud description as a fractal object, ending with the simulations of fluctuating stellar light curves.
Methods. Fast Fourier transforms are first used to simulate fractal clouds. Then, the illumination pattern resulting from the crossing of background star light through these refractive clouds is calculated from a Fresnel integral that also uses fast Fourier transform techniques. Regularisation procedure and computing limitations are discussed, along with the effect of spatial and temporal coherency (source size and wavelength passband).
Results. We quantify the expected modulation index of stellar light curves as a function of the turbulence strength – characterised by the diffraction radius Rdiff – and the projected source size, introduce the timing aspects, and establish connections between the light curve observables and the refractive cloud. We extend our discussion to clouds with different structure functions from Kolmogorov-type turbulence.
Conclusions. Our study confirms that current telescopes of ~4 m with fast-readout, wide-field detectors have the capability of discovering the first interstellar optical scintillation effects. We also show that this effect should be unambiguously distinguished from any other type of variability through the observation of desynchronised light curves, simultaneously measured by two distant telescopes.
Key words: dark matter / Galaxy: disk / Galaxy: halo / Galaxy: structure / local insterstellar matter / ISM: molecules
© ESO, 2013
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