中文
相关论文

相关论文: Subaru Spectroscopy and Spectral Modeling of Cygnu…

200 篇论文

We present 8-13 micron imaging and spectroscopy of 9 type 1 and 10 type 2 AGN obtained with the VLT/VISIR instrument at spatial resolution <100 pc. The emission from the host galaxy sources is resolved out in most cases. The silicate…

宇宙学与河外天体物理 · 物理学 2015-05-18 S. F. Hoenig , M. Kishimoto , P. Gandhi , A. Smette , D. Asmus , W. Duschl , M. Polletta , G. Weigelt

We have searched for absorption in several common atomic species due to the atmosphere or exosphere of the transiting extrasolar planet HD 209458b, using high precision optical spectra obtained with the Subaru High Dispersion Spectrograph…

We use a combination of high spatial resolution optical and near-IR spectroscopic data to make a detailed study of the kinematics of the NLR gas in the near-nuclear regions of the powerful, FRII radio galaxy Cygnus A (z=0.0560), with the…

天体物理学 · 物理学 2009-11-07 C. Tadhunter , A. Marconi , D. Axon , K. Wills , T. G. Robinson , N. Jackson

The black hole binary Cygnus X-1 was observed in late-2012 with the Nuclear Spectroscopic Telescope Array (NuSTAR) and Suzaku, providing spectral coverage over the ~1-300 keV range. The source was in the soft state with a multi-temperature…

We report Chandra ACIS and quasi-simultaneous RXTE observations of the nearby, powerful radio galaxy Cygnus A, with the present paper focusing on the properties of the active nucleus. In the Chandra observation, the hard (> a few keV) X-ray…

天体物理学 · 物理学 2009-11-07 Andrew J. Young , Andrew S. Wilson , Yuichi Terashima , Keith A. Arnaud , David A. Smith

We report X-ray observations of the powerful radio galaxy Cygnus A with the Chandra X-ray Observatory. This letter focuses on the radio hot spots, all four of which are detected in X-rays with a very similar morphology to their radio…

天体物理学 · 物理学 2009-10-31 A. S. Wilson , A. J. Young , P. L. Shopbell

We present the first detection of carbon radio recombination line absorption along the line of sight to Cygnus A. The observations were carried out with the LOw Frequency ARray in the 33 to 57 MHz range. These low frequency radio…

星系天体物理 · 物理学 2015-06-18 J. B. R. Oonk , R. J. van Weeren , F. Salgado , L. K. Morabito , A. G. G. M. Tielens , H. J. A. Rottgering , A. Asgekar , G. J. White , A. Alexov , J. Anderson , I. M. Avruch , F. Batejat , R. Beck , M. E. Bell , I. van Bemmel , M. J. Bentum , G. Bernardi , P. Best , A. Bonafede , F. Breitling , M. Brentjens , J. Broderick , M. Brueggen , H. R. Butcher , B. Ciardi , J. E. Conway , A. Corstanje , F. de Gasperin , E. de Geus , M. de Vos , S. Duscha , J. Eisloeffel , D. Engels , J. van Enst , H. Falcke , R. A. Fallows , R. Fender , C. Ferrari , W. Frieswijk , M. A. Garrett , J. Griessmeier , J. P. Hamaker , T. E. Hassall , G. Heald , J. W. T. Hessels , M. Hoeft , A. Horneffer , A. van der Horst , M. Iacobelli , N. J. Jackson , E. Juette , A. Karastergiou , W. Klijn , J. Kohler , V. I. Kondratiev , M. Kramer , M. Kuniyoshi , G. Kuper , J. van Leeuwen , P. Maat , G. Macario , G. Mann , S. Markoff , J. P. McKean , M. Mevius , J. C. A. Miller-Jones , J. D. Mol , D. D. Mulcahy , H. Munk , M. J. Norden , E. Orru , H. Paas , M. Pandey-Pommier , V. N. Pandey , R. Pizzo , A. G. Polatidis , W. Reich , A. M. M. Scaife , A. Schoenmakers , D. Schwarz , A. Shulevski , J. Sluman , O. Smirnov , C. Sobey , B. W. Stappers , M. Steinmetz , J. Swinbank , M. Tagger , Y. Tang , C. Tasse , S. ter Veen , S. Thoudam , C. Toribio , R. van Nieuwpoort , R. Vermeulen , C. Vocks , C. Vogt , R. A. M. J. Wijers , M. W. Wise , O. Wucknitz , S. Yatawatta , P. Zarka , A. Zensus

We present a comprehensive study of the silicate features at 9.7 and 18 micron of a sample of almost 800 active galactic nuclei (AGN) with available spectra from the Spitzer InfraRed Spectrograph (IRS). We measure the strength of the…

星系天体物理 · 物理学 2015-06-23 Evanthia Hatziminaoglou , Antonio Hernán-Caballero , Anna Feltre , Nuria Piñol-Ferrer

We explore the origin of mid-infrared (mid-IR) dust extinction in all 20 nearby (z < 0.05) bona-fide Compton-thick (N_H > 1.5 x 10^24 cm^-2) AGN with hard energy (E > 10 keV) X-ray spectral measurements. We accurately measure the silicate…

星系天体物理 · 物理学 2015-06-05 A. D. Goulding , D. M. Alexander , F. E. Bauer , W. R. Forman , R. C. Hickox , C. Jones , J. R. Mullaney , M. Trichas

We report the appearance of a new radio source at a projected offset of 460 pc from the nucleus of Cygnus A. The flux density of the source (which we designate Cygnus A-2) rose from an upper limit of <0.5 mJy in 1989 to 4 mJy in 2016…

高能天体物理现象 · 物理学 2017-06-02 Daniel A. Perley , Richard A. Perley , Vivek Dhawan , Christopher L. Carilli

The 10-micron silicate feature observed with Spitzer in active galactic nuclei (AGN) reveals some puzzling behavior. It (1) has been detected in emission in type 2 sources, (2) shows broad, flat-topped emission peaks shifted toward long…

宇宙学与河外天体物理 · 物理学 2011-02-11 Robert Nikutta , Moshe Elitzur , Mark Lacy

We present results of our Chandra observation with the ACIS-I instrument centered on the position of Sagittarius A* (Sgr A*), the compact nonthermal radio source associated with the massive black hole (MBH) at the dynamical center of the…

Two-dimensional radiative transfer is employed to obtain the broad-band infrared spectrum of active galaxies. In the models we vary the geometry and size of the obscuring medium, the surface density, the opacity and the grain size…

天体物理学 · 物理学 2009-11-07 I. M. van Bemmel , C. P. Dullemond

We report the detection of strong absorption and weak emission features in the 4--27 micron Spitzer-IRS spectrum of the distant ultraluminous infrared galaxy (ULIRG) IRAS F00183--7111 (z=0.327). The absorption features of CO2 and CO gas,…

This paper presents observations of Cygnus A at 74 and 327 MHz at angular resolutions of approximately 10" and 3", respectively. These observations are among the highest angular resolutions obtained below 1000 MHz for this object. While the…

天体物理学 · 物理学 2009-11-11 T. J. W. Lazio , A. S. Cohen , N. E. Kassim , R. A. Perley , W. C. Erickson , C. L. Carilli , P. C. Crane

We report the detection of linearly polarized emission at 53 and 89 $\mu$m, from the radio-loud active galactic nucleus (AGN) Cygnus A using HAWC+ onboard SOFIA. We measure a highly polarized core of $11\pm3$% and $9\pm2$% with a position…

星系天体物理 · 物理学 2018-07-25 Enrique Lopez-Rodriguez , Robert Antonucci , Ranga-ram Chary , Makoto Kishimoto

We present new imaging at 12.81 and 11.7 microns of the central ~40"x30" (~0.7x0.5 kpc) of the starburst galaxy M82. The observations were carried out with the COMICS mid-infrared (mid-IR) imager on the 8.2m Subaru telescope, and are…

星系天体物理 · 物理学 2015-05-27 P. Gandhi , N. Isobe , M. Birkinshaw , D. M. Worrall , I. Sakon , K. Iwasawa , A. Bamba

We report near-infrared K', L', and M' band imaging observations of the nearby merging galaxy NGC 6240 with the Infrared Camera and Spectrograph on the Subaru telescope. The observations were performed with the assistance of the Subaru…

We use photometric and spectroscopic infrared observations obtained with the Spitzer Space Telescope of 12 radio-loud active galactic nuclei (AGN) to investigate the dust geometry. Our approach is to look at the change of the infrared…

宇宙学与河外天体物理 · 物理学 2015-05-19 Hermine Landt , Catherine L. Buchanan , Pauline Barmby

We present deep 1.8 cm (16 GHz) radio continuum imaging of seven young stellar objects in the Taurus molecular cloud. These objects have previously been extensively studied in the sub-mm to NIR range and their SEDs modelled to provide…