Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-19T03:53:16.721Z Has data issue: false hasContentIssue false
  • English
  • Français

X-ray spectral and image spatial models of NGC 3081 with Chandra data

Published online by Cambridge University Press:  20 January 2023

O.V. Kompaniiets ,
Iu.V. Babyk Open the ORCID record for Iu.V. Babyk [Opens in a new window] ,
A.A. Vasylenko ,
I.O. Izviekova  and
I.B. Vavilova Open the ORCID record for I.B. Vavilova [Opens in a new window]
O.V. Kompaniiets
Affiliation:
Main Astronomical Observatory of the NAS of Ukraine, 27 Akademik Zabolotny Str., Kyiv, 03143, Ukraine Institute of Physics of the NAS of Ukraine, 46 av. Nauky, Kyiv, 03028, Ukraine
Iu.V. Babyk
Affiliation:
Main Astronomical Observatory of the NAS of Ukraine, 27 Akademik Zabolotny Str., Kyiv, 03143, Ukraine
A.A. Vasylenko
Affiliation:
Main Astronomical Observatory of the NAS of Ukraine, 27 Akademik Zabolotny Str., Kyiv, 03143, Ukraine
I.O. Izviekova
Affiliation:
Main Astronomical Observatory of the NAS of Ukraine, 27 Akademik Zabolotny Str., Kyiv, 03143, Ukraine ICAMER, NAS of Ukraine, 27 Akademik Zabolotny Str., Kyiv, 03143, Ukraine
I.B. Vavilova
Affiliation:
Main Astronomical Observatory of the NAS of Ukraine, 27 Akademik Zabolotny Str., Kyiv, 03143, Ukraine
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The physical properties of AGN such as accretion rate, column density, temperature of hot corona and other characteristics can be found from X-ray spectral data. We present the results of spatial and spectral analysis for Sy2 type galaxy NGC 3081 obtained with different mathematical tools of the Chandra Interactive Analysis of Observations software. We found evidence of extended emission in 0.5-3.0 keV as well as derived parameters for model A: photon index , column density , warm component and hot component . We detected the presence of a component of the reflection spectrum, Fe Kα emission line with and .

Keywords

methods: data analysisgalaxies: active galactic nucleiNGC 3081
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 16 , Symposium S362: The Predictive Power of Computational Astrophysics as a Discovery Tool , June 2020 , pp. 100 - 104
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Antonucci, R., Miller, J. 1985, ApJ, 297, 621 CrossRefGoogle Scholar
Chesnok, N.G., Sergeev, S.G., Vavilova, I.B. 2009, Kinemat. Physics Celest. Bodies, 25, 107.CrossRefGoogle Scholar
Doe, S., Nguyen, D., Stawarz, C. et al. 2007, ADASS XVI, 376, 543.Google Scholar
Freeman, P., Doe, S., Siemiginowska, A. 2001, Astronomical Data Analysis, 4477, 76.Google Scholar
Gross, A. et al. 2019, AAS Meeting Abstracts, #233.Google Scholar
Guainazzi, M., De Rosa, A., Bianchi, S. et al. 2021, MNRAS, 504, 393.Google Scholar
Haardt, F., Maraschi, L. 1991, ApJ, 380, 51 CrossRefGoogle Scholar
Haardt, F., Maraschi, L. 1993, ApJ, 413, 507 CrossRefGoogle Scholar
Jin, G., Dai, Y.S., Pan, H.A. et al. 2021, Astrophys. J., 923, 6.CrossRefGoogle Scholar
Karachentseva, V.E. and Vavilova, I.B. 1994, Bull.Special Astrophys. Observatory 37, 98.Google Scholar
Karachentseva, V.E. and Vavilova, I.B. 1995, Kinemat. Phys. Celestial Bodies 11, 38.Google Scholar
Karachentseva, V.E., Mitronova, S.N., Melnyk, O.V. et al 2010, Astrophys. Bull., 65, 1.CrossRefGoogle Scholar
Kompaniiets, O.V. & Vasylenko, A.A. 2020, Astrophysics, 63, 307.CrossRefGoogle Scholar
Mushotzky, R.F., Done, C., Pounds, K.A. 1993 Annual Rev. Astron. Astrophys. 31, 717CrossRefGoogle Scholar
Pulatova, N.G., Vavilova, I.B., Sawangwit, U., et al. 2015, Mon. Not. R. Astron. Soc., 447, 3, 2209.CrossRefGoogle Scholar
Ramos, A.C. & Ricci, C. 2017, Nature Astronomy, 1, 679.Google Scholar
Schnorr-Müller, A. et al. 2016, MNRAS, 457, 972.CrossRefGoogle Scholar
Smirnova, A.A., Moiseev, A.V., Afanasiev, V.L. 2010, Hunting for the Dark: the Hidden Side of Galaxy Formation, 1240, 297.Google Scholar
Vasylenko, A.A., Vavilova, I.B., Pulatova, N.G. 2020, Astron. Nachr., 341, 8, 801.CrossRefGoogle Scholar
Vavilova, I.B., Karachentseva, V.E., Makarov, D.I., and Melnyk, O.V. 2005, Kinemat. Fiz. Nebesnykh Tel 21, 3.Google Scholar
Vavilova, I.B., Vasylenko, A.A., Babyk, Iu.V., Pulatova, N.G. 2015, Odessa Astron. Publ., 28(2), 150.CrossRefGoogle Scholar
Véron-Cetty, M.P., Véron, P. 2010, Astron. Astrophys., 518, A10.CrossRefGoogle Scholar
Vol’Vach, A.E., Vol’Vach, L.N., Kut’kin, A.M. et al. 2011, Astron. Reports 55, 608.CrossRefGoogle Scholar