Near infrared flares of Sagittarius A*: Importance of near infrared polarimetry
M. Zamaninasab, A. Eckart, G. Witzel, M. Dovciak, V. Karas, R., Schoedel R. Giessuebel, M. Bremer, M. Garcia-Marin, D. Kunneriath, K. Muzic,, S. Nishiyama, N. Sabha, C. Straubmeier, A. Zensus

TL;DR
This paper presents simulations and observations of near-infrared flares from Sagittarius A*, emphasizing the importance of polarimetry in understanding accretion processes and detecting orbiting matter near the black hole.
Contribution
It introduces a combined approach of simulations and multi-epoch observations to analyze NIR flares and polarization, confirming the hot spot model and detecting signatures of orbiting matter.
Findings
Correlation between flux modulations and polarization changes
Detection of orbiting matter signatures under strong gravity
Confirmation of hot spot model predictions
Abstract
We report on the results of new simulations of near-infrared (NIR) observations of the Sagittarius A* (Sgr A*) counterpart associated with the super-massive black hole at the Galactic Center. The observations have been carried out using the NACO adaptive optics (AO) instrument at the European Southern Observatory's Very Large Telescope and CIAO NIR camera on the Subaru telescope (13 June 2004, 30 July 2005, 1 June 2006, 15 May 2007, 17 May 2007 and 28 May 2008). We used a model of synchrotron emission from relativistic electrons in the inner parts of an accretion disk. The relativistic simulations have been carried out using the Karas-Yaqoob (KY) ray-tracing code. We probe the existence of a correlation between the modulations of the observed flux density light curves and changes in polarimetric data. Furthermore, we confirm that the same correlation is also predicted by the hot spot…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Mechanics and Biomechanics Studies · Pulsars and Gravitational Waves Research
