Compton-Thick AGN in the NuSTAR era VIII: A joint NuSTAR-XMM-Newton monitoring of the changing-look Compton-thick AGN NGC 1358
| Autor: | Marchesi, Stefano, Zhao, Xiurui, Torres-Albà, Núria, Ajello, Marco, Gaspari, Massimo, Pizzetti, Andrealuna, Buchner, Johannes, Bertola, Elena, Comastri, Andrea, Feltre, Anna, Gilli, Roberto, Lanzuisi, Giorgio, Matzeu, Gabriele, Pozzi, Francesca, Salvestrini, Francesco, Sengupta, Dhrubojyoti, Silver, Ross, Tombesi, Francesco, Traina, Alberto, Vignali, Cristian, Zappacosta, Luca |
|---|---|
| Rok vydání: | 2022 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| DOI: | 10.3847/1538-4357/ac80be |
| Popis: | We present the multi-epoch monitoring with NuSTAR and XMM-Newton of NGC 1358, a nearby Seyfert 2 galaxy whose properties made it a promising candidate X-ray changing look AGN, i.e., a source whose column density could transition from its 2017 Compton-thick (CT-, having line-of-sight Hydrogen column density NH,los>10^24 cm^-2) state to a Compton-thin (NH,los<10^24 cm^-2) one. The multi-epoch X-ray monitoring confirmed the presence of significant NH,los variability over time-scales as short as weeks, and allowed us to confirm the "changing look" nature of NGC 1358, which has most recently been observed in a Compton-thin status. Multi-epoch monitoring with NuSTAR and XMM-Newton is demonstrated to be highly effective in simultaneously constraining three otherwise highly degenerate parameters: the torus average column density and covering factor, and the inclination angle between the torus axis and the observer. We find a tentative anti-correlation between column density and luminosity, which can be understood in the framework of Chaotic Cold Accretion clouds driving recursive AGN feedback. The monitoring campaign of NGC 1358 has proven the efficiency of our newly developed method to select candidate NH,los-variable, heavily obscured AGN, which we plan to soon extend to a larger sample to better characterize the properties of the obscuring material surrounding accreting supermassive black holes, as well as constrain AGN feeding models. Comment: 24 pages, 13 figures: main results in Figures 4, 7, 8 and 9. Accepted for publication in the Astrophysical Journal |
| Databáze: | arXiv |
| Externí odkaz: |
|