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Gaseous environment in LLAGN: modes of interaction with compact star nuclear population

  • M. Zajaček (a1) (a2), V. Karas (a1), L. Šubr (a2), D. Kunneriath (a1) and A. Eckart (a3) (a4)...

Abstract

The Galactic center, which serves as a paradigm of low-luminosity active galactic nuclei (LLAGN), hosts the Nuclear star cluster (NSC) that contains both young and more evolved stars. So far the population of the end-products of stellar evolution has not been observationally confirmed and studied, although there are hints of its presence. We study the distribution of interaction modes of a hypothetical population of neutron stars within the sphere of influence of the Sgr A* supermassive black hole (SMBH). The comparison of our models with future observations could be used to constrain the 3D structure of the Galactic center.

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References

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Kunneriath, D., Eckart, A., Vogel, S. N., et al., 2012, A&A, 538, A127
Morris, M., 1993, ApJ, 408, 496
Zajaček, M., 2014a, MSc. Thesis, Charles University in Prague, Czech Republic
Zajaček, M., Karas, V., Kunneriath, D., 2014b, Proc. of IBWS 2014, Acta Polytechnica, submitted
Zhao, J.-H., Blundell, R., Moran, J. M., et al., 2010, ApJ, 723, 1097
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Gaseous environment in LLAGN: modes of interaction with compact star nuclear population

  • M. Zajaček (a1) (a2), V. Karas (a1), L. Šubr (a2), D. Kunneriath (a1) and A. Eckart (a3) (a4)...

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