دورية أكاديمية

Space Telescope and Optical Reverberation Mapping Project. X. Understanding the Absorption-line Holiday in NGC 5548 ; Astrophysical Journal

التفاصيل البيبلوغرافية
العنوان: Space Telescope and Optical Reverberation Mapping Project. X. Understanding the Absorption-line Holiday in NGC 5548 ; Astrophysical Journal
المؤلفون: Dehghanian, M., Ferland, G. J., Kriss, G. A., Peterson, B. M., Mathur, S., Mehdipour, M., Guzman, F., Chatzikos, M., van Hoof, P. A. M., Williams, R. J. R., Arav, Nahum, Barth, A. J., Bentz, M. C., Bisogni, S., Brandt, W. N., Crenshaw, D. M., Dalla Bonta, E., De Rosa, G., Fausnaugh, M. M., Gelbord, J. M., Goad, M. R., Gupta, A., Horne, Keith, Kaastra, J., Knigge, C., Korista, K. T., McHardy, I. M., Pogge, R. W., Starkey, D. A., Vestergaard, M.
المساهمون: Physics
سنة النشر: 2019
المجموعة: VTechWorks (VirginiaTech)
مصطلحات موضوعية: galaxies: active, galaxies: individual (NGC 5548), galaxies: nuclei, galaxies: Seyfert, line: formation
الوصف: The Space Telescope and Optical Reverberation Mapping Project (AGN STORM) on NGC 5548 in 2014 is one of the most intensive multiwavelength AGN monitoring campaigns ever. For most of the campaign, the emission-line variations followed changes in the continuum with a time lag, as expected. However, the lines varied independently of the observed UV-optical continuum during a 60-70 day "holiday," suggesting that unobserved changes to the ionizing continuum were present. To understand this remarkable phenomenon and to obtain an independent assessment of the ionizing continuum variations, we study the intrinsic absorption lines present in NGC 5548. We identify a novel cycle that reproduces the absorption line variability and thus identify the physics that allows the holiday to occur. In this cycle, variations in this obscurer's line-of-sight covering factor modify the soft X-ray continuum, changing the ionization of helium Ionizing radiation produced by recombining helium then affects the level of ionization of some ions seen by the Hubble Space Telescope. In particular, high-ionization species are affected by changes in the obscurer covering factor, which does not affect the optical or UV continuum, and thus appear as uncorrelated changes, a "holiday." It is likely that any other model that selectively changes the soft X-ray part of the continuum during the holiday can also explain the anomalous emission-line behavior observed. ; NASA through a grant from the Space Telescope Science Institute [NNX15AH49G, 80NSSC17K0126, NAS5-26555]; NSF [1816537, AST-1816537, AST-1412693, AST-1009756, AST-1412315]; NASA [NNX15AH49G, 80NSSC17K0126, ATP 17-0141, AR7-18013X, NAS8-03060, PF5-160141]; STScI [HST-AR.13914, HST-AR-15018]; NASA through STScI grant [HST-AR-14556.001A, HST-AR-14286]; Huffaker Scholarship; National Science Foundation [AST-1008882]; NSF CAREER [AST-1253702]; Padua University [DOR1699945/16, DOR1715817/17, DOR1885254/18, BIRD164402/16]; NSF Fellowship award [AST-1302093]; STFC [ST/R000824/1, ST/M001326/1]; NWO; ...
نوع الوثيقة: article in journal/newspaper
still image
وصف الملف: application/pdf
اللغة: English
تدمد: 0004-637X
1538-4357
العلاقة: 119; http://hdl.handle.net/10919/93242Test; https://doi.org/10.3847/1538-4357/ab1b48Test; 877
DOI: 10.3847/1538-4357/ab1b48
الإتاحة: https://doi.org/10.3847/1538-4357/ab1b48Test
http://hdl.handle.net/10919/93242Test
حقوق: Creative Commons Attribution 3.0 Unported ; http://creativecommons.org/licenses/by/3.0Test/
رقم الانضمام: edsbas.7C144AD
قاعدة البيانات: BASE
الوصف
تدمد:0004637X
15384357
DOI:10.3847/1538-4357/ab1b48