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相关论文: Polarization and kinematics in Cygnus A

200 篇论文

The results from a recent Chandra ACIS-S study of the cluster surrounding Cygnus A are presented. We have deprojected the X-ray spectra taken from various elliptical shells in order to derive the run of temperature, density, pressure, and…

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

We present near-infrared broad-band polarization images of the nuclear regions of the Circinus galaxy in the J, H and K bands. For the first time the south-eastern reflection cone is detected in polarized light, which is obscured at optical…

天体物理学 · 物理学 2009-10-31 M. Ruiz , D. M. Alexander , S. Young , J. Hough , S. L. Lumsden , C. A. Heisler

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

Context: Most active galactic nuclei (AGN) are believed to be surrounded by a dusty molecular torus on the parsec scale which is often embedded within a larger circumnuclear disk (CND). AGN are fuelled by the inward transport of material…

We report results from broadband visible images of comet C/2012 S1 (ISON) obtained with the Hubble Space Telescope Wide Field Camera 3 on 2013 April 10. C/ISON's coma brightness follows a 1/{\rho} (where {\rho} is the projected distance…

Even when the direct view toward the active nucleus is obscured, nuclear emission propagating along other directions can scatter off surrounding material, become polarized and reach the observer. Spectropolarimetry can thus be an important…

星系天体物理 · 物理学 2023-09-06 Nadia L. Zakamska , Rachael M. Alexandroff

We characterize the physical properties of the cool T ~10^4 K circumgalactic medium surrounding z ~2-3 quasar host galaxies, which are predicted to evolve into present day massive ellipticals. Using a statistical sample of 14 quasar pairs…

星系天体物理 · 物理学 2016-10-26 Marie Wingyee Lau , J. Xavier Prochaska , Joseph F. Hennawi

We present the first direct imaging of what may be the thick torus in the active galactic nucleus (AGN) of the archetype powerful radio galaxy Cygnus A, using the Jansky Very Large Array (VLA) at 18 GHz to 48 GHz, with a resolution down to…

高能天体物理现象 · 物理学 2019-07-17 C. L. Carilli , R. A. Perley , V. Dhawan , D. A. Perley

(Abridged) Complex organic molecules (COMs) are commonly detected in and near star-forming regions. However, the dominant process in the release of these COMs from the icy grains - where they predominately form - to the gas phase is still…

太阳与恒星天体物理 · 物理学 2021-11-24 S. J. van der Walt , L. E. Kristensen , J. K. Jørgensen , H. Calcutt , S. Manigand , M. el Akel , R. T. Garrod , K. Qiu

We present results from deep, wideband, high spatial and spectral resolution observations of the nearby luminous radio galaxy Cygnus A with the Jansky Very Large Array. The high surface brightness of this source enables detailed…

Recent mid-infrared interferometry observations of nearby active galactic nuclei (AGN) revealed that a significant part of the dust emission extends in the polar direction, rather than the equatorial torus/disk direction as expected by the…

高能天体物理现象 · 物理学 2019-11-06 Jiren Liu , Sebastian F. Hönig , Claudio Ricci , Stéphane Paltani

We report a polarimetric constraint on the hard X-ray synchrotron jet emission from the Cygnus X-1 black-hole binary system. The observational data were obtained using the PoGO+ hard X-ray polarimeter in July 2016, when Cygnus X-1 was in…

We report on a discovery of a diffuse nebula containing a pointlike source in the southern blowout region of the Cygnus Loop supernova remnant, based on Suzaku and XMM-Newton observations. The X-ray spectra from the nebula and the pointlike…

高能天体物理现象 · 物理学 2015-06-05 Satoru Katsuda , Hiroshi Tsunemi , Koji Mori , Hiroyuki Uchida , Robert Petre , Shin'ya Yamada , Toru Tamagawa

We present H-alpha and [O III] (5007 Angstroms) images of the nebula powered by the jet of the black hole candidate and microquasar Cygnus X-1, observed with the 2.5m Isaac Newton Telescope (INT). The ring-like structure is luminous in [O…

天体物理学 · 物理学 2008-11-26 D. M. Russell , R. P. Fender , E. Gallo , C. R. Kaiser

We present new observations of the [Ne II] emission from the ionized gas in Sgr A West with improved resolution and sensitivity. About half of the emission comes from gas with kinematics indicating it is orbiting in a plane tipped about…

星系天体物理 · 物理学 2015-06-05 Wesley T. Irons , John H. Lacy , Matthew J. Richter

If Type-II supernovae - the evolutionary end points of short-lived, massive stars - produce a significant quantity of dust (>0.1 M_sun) then they can explain the rest-frame far-infrared emission seen in galaxies and quasars in the first Gyr…

Results of 2D spectral observations for 4 Sy galaxies with ionization cones are presented. Images in the [OIII] line, velocity fields of the ionized gas, stellar velocity and velocity dispersion fields were obtained at the SAO RAS 6m…

天体物理学 · 物理学 2007-05-23 A. V. Moiseev , V. L. Afanasiev , S. N. Dodonov , V. V. Mustsevoi , S. S. Khrapov

Red quasars, often associated with potent [OIII] outflows on both galactic and circumgalactic scales, may play a pivotal role in galactic evolution and black hole feedback. In this work, we explore the [FeII] emission in one such quasar at…

We summarize recent observations of Cyg X-1 during its 1996 state transition. The results favor an emission geometry with a central optically thin corona surrounded by an optically thick, geometrically thin accretion disk. As the soft state…

天体物理学 · 物理学 2007-05-23 Wei Cui , S. N. Zhang , J. H. Swank , X. -M. Hua , K. Ebisawa , T. Dotani

Ninety per cent of baryons are located outside galaxies, either in the circumgalactic or intergalactic medium. Theory points to galactic winds as the primary source of the enriched and massive circumgalactic medium. Winds from compact…