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

Published online by Cambridge University Press:  09 February 2015

M. Zajaček ,
V. Karas ,
L. Šubr ,
D. Kunneriath  and
A. Eckart
M. Zajaček
Affiliation:
Academy of Sciences, Boční II 1401, CZ-14100Prague, Czech Republic email: michal.zajacek31@gmail.com Charles University in Prague, V Holešovičkách 2, CZ-18000Prague, Czech Republic
V. Karas
Affiliation:
Academy of Sciences, Boční II 1401, CZ-14100Prague, Czech Republic email: michal.zajacek31@gmail.com
L. Šubr
Affiliation:
Charles University in Prague, V Holešovičkách 2, CZ-18000Prague, Czech Republic
D. Kunneriath
Affiliation:
Academy of Sciences, Boční II 1401, CZ-14100Prague, Czech Republic email: michal.zajacek31@gmail.com
A. Eckart
Affiliation:
Universität zu Köln, Zülpicher Strasse 77, D-50937Köln, Germany MPIfR, Auf dem Hügel 69, D-53121 Bonn, Germany
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Abstract

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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.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 353
Copyright
Copyright © International Astronomical Union 2015 

References

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