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相关论文: Ultraviolet Lines and Gas Composition in NGC 1068

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Previous X-ray and ultraviolet spectroscopy suggested that the Fe/O abundance ratio in NGC 1068 may be abnormally high. We have measured some 15 X-ray lines in NGC 1068, to an accuracy better than a factor 2, and modeled the continuum in…

天体物理学 · 物理学 2009-10-30 Hagai Netzer , J. Turner

The physical conditions in the inner narrow line region (NLR) of the Seyfert 2 galaxy, NGC 1068, are examined using ultraviolet and optical spectra and photoionization models. The spectra are Hubble Space Telescope (HST) Harchive data…

天体物理学 · 物理学 2009-10-30 Steven B. Kraemer , Jose R. Ruiz , D. Michael Crenshaw

We present a detailed, photoionization modeling analysis of XMM-Newton/Reflection Grating Spectrometer observations of the Seyfert 2 galaxy NGC 1068. The spectrum, previously analyzed by Kinkhabwala et al. (2002), reveals a myriad of…

星系天体物理 · 物理学 2015-06-23 S. B. Kraemer , N. Sharma , T. J. Turner , Ian M. George , D. Michael Crenshaw

The first complete far-infrared spectrum (43-197um) of the Seyfert 2 galaxy NGC 1068 as observed with the LWS onboard ISO is reported. In addition to the expected ionic fine structure emission lines, the OH rotational lines at 79, 119 and…

We present ISO-SWS spectroscopy of NGC 1068 for the wavelength range 2.4 to 45um, detecting a total of 36 emission lines. Most of the observed transitions are fine structure and recombination lines originating in the narrow line region. We…

天体物理学 · 物理学 2009-10-31 D. Lutz , E. Sturm , R. Genzel , A. F. M. Moorwood , T. Alexander , H. Netzer , A. Sternberg

We present fully sampled ^{12}$CO, ^{13}CO J=2-1, 3-2 maps of the inner $\sim 1'\times 1'$ region of NGC 1068. We combine these measurements with an existing interferometric map of ^{12}CO J=1-0 that includes single dish data and thus…

天体物理学 · 物理学 2009-10-31 Padeli. P. Papadopoulos , E. R. Seaquist

An imaging survey of CO(1-0), HCN(1-0), and HCO$^+$(1-0) lines in the centers of nearby Seyfert galaxies has been conducted using the Nobeyama Millimeter Array and the RAINBOW interferometer. Preliminary results reveal that 3 Seyferts out…

天体物理学 · 物理学 2007-05-23 K. Kohno , S. Matsushita , B. Vila-Vilaro , S. K. Okumura , T. Shibatsuka , M. Okiura , S. Ishizuki , R. Kawabe

There is observational evidence that nuclear winds and X-rays can heavily influence the physical conditions and chemical abundances of molecular gas in the circumnuclear disks (CND) of Active Galactic Nuclei (AGN). In this paper we probe…

天体物理学 · 物理学 2009-11-10 A. Usero , S. Garcia-Burillo , A. Fuente , J. Martin-Pintado , N. J. Rodriguez-Fernandez

We present J-band long-slit spectroscopic observation of NGC 1068 classified as a Seyfert 2 galaxy. J-band observations with OAO/ISLE provide clear detection of spatially extended [Fe II]1.257um and [P II]1.188um lines. We found that [Fe…

宇宙学与河外天体物理 · 物理学 2015-05-20 Tetsuya Hashimoto , Tohru Nagao , Kenshi Yanagisawa , Kenta Matsuoka , Nobuo Araki

We investigated the kinematic and excitation structure of the NGC 1068 narrow-line region (NLR). We obtained profiles of several emission lines, [OIII]$\lambda$5007, H$\beta$, [OI]$\lambda$6300 and [FeVII]$\lambda$6087 at high-velocity…

星系天体物理 · 物理学 2015-05-13 Shinobu Ozaki

(abridged) Based on observations of the Seyfert nucleus in NGC1068 with ASCA, RXTE and BeppoSAX, we report the discovery of a flare (increase in flux by a factor of ~1.6) in the 6.7 keV Fe K line component between observations obtained 4…

天体物理学 · 物理学 2009-11-07 Edward Colbert , Kim Weaver , Julian Krolik , John Mulchaey , Richard Mushotzky

We present and discuss the high energy (E>4 keV) XMM-Newton spectrum of the Seyfert 2 galaxy, NGC 1068. Possible evidence for flux variability in both the neutral and ionized reflectors with respect to a BeppoSAX observation taken 3.5 years…

天体物理学 · 物理学 2009-11-10 Giorgio Matt , Stefano Bianchi , Matteo Guainazzi , Silvano Molendi

The ISO-SWS 2.5-45 um infrared spectroscopic observations of the nucleus of the Seyfert 2 galaxy NGC 1068 (see companion paper) are combined with a compilation of UV to IR narrow emission line data to determine the spectral energy…

天体物理学 · 物理学 2009-10-31 Tal Alexander , Dieter Lutz , Eckhard Sturm , Reinhard Genzel , Amiel Sternberg , Hagai Netzer

We present ultraviolet emission-line maps of the narrow-line region (NLR) of NGC 1068. The maps span 115--318 nm, the biconical ionization cone, several posited jet/ISM interactions, and the compact knots whose optical spectra we reported…

天体物理学 · 物理学 2008-11-26 Brent Groves , Gerald Cecil , Pierre Ferruit , Michael Dopita

We report sub arc-second resolution X-ray imaging-spectroscopy of the archetypal type 2 Seyfert galaxy NGC 1068 with the Chandra X-ray Observatory. The observations reveal the detailed structure and spectra of the 13 kpc-extent nebulosity…

天体物理学 · 物理学 2009-11-06 A. J. Young , A. S. Wilson , P. L. Shopbell

Aims. We investigate the physical and chemical conditions of molecular gas in the circumnuclear disk (CND) region of NGC 1068. Methods. We carried out a spectral line survey with the IRAM 30m telescope toward the center of NGC 1068 and…

星系天体物理 · 物理学 2020-02-26 Jianjie Qiu , Jiangshui Zhang , Yong Zhang , Lanwei Jia , Xindi Tang

The physical conditions in the inner narrow line region (NLR) of the Seyfert 2 galaxy NGC 1068 are examined using HST/STIS ultraviolet and optical spectra and photoionization models. 1) The emission-line gas in the blueshifted northeast…

天体物理学 · 物理学 2009-10-31 Steven B. Kraemer , D. Michael Crenshaw

We use the full broad-band XMM-Newton EPIC data to examine the X-ray spectrum of the nearby Seyfert 2 galaxy NGC 1068, previously shown to be complex with the X-ray continuum being a sum of components reflected/scattered from cold (neutral)…

天体物理学 · 物理学 2009-11-11 K. Pounds , S. Vaughan

We present high angular resolution (0.5-2.0") observations of the mm continuum and the 12CO(J=3-2), 13CO(J=3-2), 13CO(J=2-1), C18O(J=2-1), HCN(J=3-2), HCO+(J=4-3) and HCO+(J=3-2) line emission in the circumnuclear disk (r=100pc) of the…

We investigate the far infrared spectrum of NGC 1266, a S0 galaxy that contains a massive reservoir of highly excited molecular gas. Using the SPIRE-FTS, we detect the $^{12}$CO ladder up to J=(13-12), [C I] and [N II] lines, and also…

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