Near Infrared Polarimetry as a Tool for Testing the Properties of Radiation from Sagittarius A*

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Our goal is to investigate and understand the physical processes behind the variability associated with the NIR flaring emission from Sagittarius A* (Sgr A*). We found a correlation between the modulations of the observed flux density light curves and changes in polarimetric data. Correlations between intensity and polarimetric parameters of the observed light curves as well as a comparison of predicted and observed light curve features through a panttern recognition algorithm resulted in the detection of a signature of orbiting matter under the influence of strong gravity. This pattern is detected statistically significant against randomly polarized red noise.

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