HST/COS observations of the newly discovered obscuring outflow in NGC3783

被引:22
作者
Kriss, G. A. [1 ]
Mehdipour, M. [2 ]
Kaastra, J. S. [2 ,3 ]
Rau, A. [4 ]
Bodensteiner, J. [4 ,5 ]
Plesha, R. [1 ]
Arav, N. [6 ]
Behar, E. [7 ]
Bianchi, S. [8 ]
Branduardi-Raymont, G. [9 ]
Cappi, M. [10 ]
Costantini, E. [2 ]
De Marco, B. [11 ]
Di Gesu, L. [12 ]
Ebrero, J. [13 ]
Kaspi, S. [7 ]
Mao, J. [2 ,3 ]
Middei, R. [8 ]
Miller, T. [6 ]
Paltani, S. [12 ]
Peretz, U. [7 ]
Peterson, B. M. [1 ,14 ,15 ]
Petrucci, P. -O. [16 ]
Ponti, G. [17 ]
Ursini, F. [10 ]
Walton, D. J. [18 ]
Xu, X. [6 ]
机构
[1] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[2] SRON Netherlands Inst Space Res, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands
[3] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands
[4] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany
[5] Katholieke Univ Leuven, Inst Astron, Celestijnenlaan 200D Bus 2401, B-3001 Leuven, Belgium
[6] Virginia Tech, Dept Phys, Blacksburg, VA 24061 USA
[7] Technion Israel Inst Technol, Dept Phys, IL-32000 Haifa, Israel
[8] Univ Roma Tre, Dipartimento Matemat & Fis, Via Vasca Navale 84, I-00146 Rome, Italy
[9] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[10] INAF IASF Bologna, Via Gobetti 101, I-40129 Bologna, Italy
[11] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland
[12] Univ Geneva, Dept Astron, 16 Ch Ecogia, CH-1290 Versoix, Switzerland
[13] European Space Astron Ctr, POB 78, Madrid 28691, Spain
[14] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA
[15] Ohio State Univ, Ctr Cosmol & AstroParticle Phys, 191 West Woodruff Ave, Columbus, OH 43210 USA
[16] Univ Grenoble Alpes, CNRES, IPAG, F-38000 Grenoble, France
[17] Osserv Astron Brera, INAF, Via E Bianchi 46, I-23807 Merate, LC, Italy
[18] Inst Astron, Madingley Rd, Cambridge CB3 0HA, England
基金
欧盟地平线“2020”;
关键词
ultraviolet: galaxies; galaxies: active; galaxies: Seyfert; galaxies: individual: NGC3783; quasars: absorption lines; quasars: emission lines; ACTIVE GALACTIC NUCLEI; BROAD-LINE REGION; SUPERMASSIVE BLACK-HOLES; REVERBERATION MAPPING DATA; RADIO-QUIET QUASARS; IONIZED-GAS; DISK WINDS; ULTRAVIOLET CONTINUUM; ENVIRONMENT; VARIABILITY;
D O I
10.1051/0004-6361/201834326
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. To understand the nature of transient obscuring outflows in active galactic nuclei, we use simultaneous multiwavelength observations with XMM-Newton, NuSTAR, the Hubble Space Telescope (HST), and the Max Planck Gesellschaft/European Southern Observatory (ESO) 2.2 m telescope triggered by soft X-ray absorption detected by Swift. Methods. We obtained ultraviolet spectra on 2016-12-12 and 2016-12-21 using the Cosmic Origins Spectrograph (COS) on HST simultaneously with X-ray spectra obtained with XMM-Newton and NuSTAR. We modeled the ultraviolet spectra to measure the strength and variability of the absorption, and used photoionization models to obtain its physical characteristics. Results. We find new components of broad, blue-shifted absorption associated with Ly alpha, N v, Si IV, and C IV in our COS spectra. The absorption extends from near-zero velocities in the rest-frame of the host galaxy to -6200 km s(-1). These features appear for the first time in NGC3783 at the same time as heavy soft X-ray absorption seen in the XMM-Newton X-ray spectra. The X-ray absorption has a column density of similar to 10(23) cm(-2), and it partially covers the X-ray continuum source. Combining the X-ray column densities with the UV spectral observations yields an ionization parameter for the obscuring gas of log xi = 1.84(-0.2)(+0.4)erg cm s(-1). Despite the high intensity of the UV continuum in NGC3783, F(1470 angstrom) = 8 x 10(-14) erg cm(-2) s(-1) angstrom(-1), the well known narrow UV absorption lines are deeper than in earlier observations in unobscured states, and low ionization states such as C III appear, indicating that the narrow-line gas is more distant from the nucleus and is being shadowed by the gas producing the obscuration. Despite the high continuum flux levels in our observations of NGC3783, moderate velocities in the UV broad line profiles have substantially diminished. Conclusions. We suggest that a collapse of the broad line region has led to the outburst and triggered the obscuring event.
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页数:24
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