Constraints on the Mass Accretion Rate onto the Supermassive Black Hole of Cygnus A Using the Submillimeter Array
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P. Koch | P. Ho | J. Algaba | M. Inoue | G. Bower | K. Akiyama | K. Asada | H. Pu | J. Koay | S. Koyama | W. Lo | S. Matsushita | Masanori Nakamura | R. Rao | Chihyin Tseng | M. Nakamura | Wen-Ping Lo | Hung-Yi Pu
[1] M. Kino,et al. Faraday Rotation in the Jet of M87 inside the Bondi Radius: Indication of Winds from Hot Accretion Flows Confining the Relativistic Jet , 2018, The Astrophysical Journal.
[2] J. Algaba,et al. Parabolic Jets from the Spinning Black Hole in M87 , 2018, The Astrophysical Journal.
[3] H. Falcke,et al. ALMA Polarimetry of Sgr A*: Probing the Accretion Flow from the Event Horizon to the Bondi Radius , 2018, The Astrophysical Journal.
[4] R. Chary,et al. The Highly Polarized Dusty Emission Core of Cygnus A , 2018, The Astrophysical Journal.
[5] C. Carilli,et al. The Cocoon Shocks of Cygnus A: Pressures and Their Implications for the Jets and Lobes , 2018, 1802.10106.
[6] Fast-spinning Black Holes Inferred from Symmetrically Limb-brightened Radio Jets , 2018, The Astrophysical Journal.
[7] J. Ostriker,et al. Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics. II. High Angular Momentum Case , 2017, The Astrophysical Journal.
[8] L. Ho,et al. Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics. I. Low Angular Momentum Case , 2018 .
[9] S. Longmore,et al. A 1.3 mm SMA Survey of 29 Variable Young Stellar Objects , 2017, 1710.08686.
[10] R. Plambeck,et al. What Is the Hidden Depolarization Mechanism in Low-luminosity AGNs? , 2017, 1707.00066.
[11] R. Lico,et al. Interpreting the time variable RM observed in the core region of the TeV blazar Mrk 421 , 2017, 1704.06133.
[12] G. Pisano,et al. Polarimetry at millimeter wavelengths with the NIKA camera: Calibration and performance , 2016, 1609.02042.
[13] J. A. Zensus,et al. First 3 mm-VLBI imaging of the two-sided jet in Cygnus A - Zooming into the launching region , 2016, 1603.04221.
[14] Christina Freytag,et al. Radiative Processes In Astrophysics , 2016 .
[15] K. Menten,et al. THE ENVIRONMENT OF THE STRONGEST GALACTIC METHANOL MASER , 2015, 1503.06841.
[16] R. Narayan,et al. NUMERICAL SIMULATION OF HOT ACCRETION FLOWS. III. REVISITING WIND PROPERTIES USING THE TRAJECTORY APPROACH , 2015, 1501.01197.
[17] M. Johnson,et al. PROBING THE PARSEC-SCALE ACCRETION FLOW OF 3C 84 WITH MILLIMETER WAVELENGTH POLARIMETRY , 2014, 1410.5887.
[18] E. Perlman,et al. POLARIZED MID-INFRARED SYNCHROTRON EMISSION IN THE CORE OF CYGNUS A , 2014, 1407.6365.
[19] A. Tchekhovskoy,et al. On the efficiency of jet production in radio galaxies , 2014, 1406.7420.
[20] A. Tchekhovskoy,et al. Dynamically important magnetic fields near accreting supermassive black holes , 2014, Nature.
[21] P. Koch,et al. MEASURING MASS ACCRETION RATE ONTO THE SUPERMASSIVE BLACK HOLE IN M87 USING FARADAY ROTATION MEASURE WITH THE SUBMILLIMETER ARRAY , 2014, 1402.5238.
[22] R. Narayan,et al. Hot Accretion Flows Around Black Holes , 2014, 1401.0586.
[23] R. Narayan,et al. Energy, momentum and mass outflows and feedback from thick accretion discs around rotating black holes , 2013, 1307.1143.
[24] Harvard,et al. Efficient Generation of Jets from Magnetically Arrested Accretion on a Rapidly Spinning Black Hole , 2011, 1108.0412.
[25] Cambridge,et al. Bondi flow from a slowly rotating hot atmosphere , 2011, 1105.0594.
[26] Stephen R. Green,et al. Numerical parameter survey of non‐radiative black hole accretion: flow structure and variability of the rotation measure , 2010, 1011.5498.
[27] P. Nulsen,et al. ARE RADIO ACTIVE GALACTIC NUCLEI POWERED BY ACCRETION OR BLACK HOLE SPIN? , 2010, 1007.1227.
[28] A. Fabian,et al. The power output of local obscured and unobscured AGN: crossing the absorption barrier with Swift/ BAT and IRAS , 2009, 0910.5256.
[29] Paul S. Smith,et al. Multiwaveband Polarimetric Observations of 15 Active Galactic Nuclei at High Frequencies: Correlated Polarization Behavior , 2007, 0705.4273.
[30] J. M. Moran,et al. Interferometric Measurements of Variable 340 GHz Linear Polarization in Sagittarius A* , 2005, astro-ph/0511653.
[31] M. Wright,et al. The Hot Spots of Cygnus A at 230 GHz , 2004 .
[32] J. Krolik,et al. Magnetically Driven Accretion Flows in the Kerr Metric. II. Structure of the Magnetic Field , 2003, astro-ph/0311500.
[33] A. Marconi,et al. Spectroscopy of the near-nuclear regions of Cygnus A: estimating the mass of the supermassive black hole , 2003, astro-ph/0302513.
[34] Geoffrey C. Bower,et al. Interferometric Detection of Linear Polarization from Sagittarius A* at 230 GHz , 2003, astro-ph/0302227.
[35] R. Narayan,et al. Three-dimensional Magnetohydrodynamic Simulations of Spherical Accretion , 2001, astro-ph/0105365.
[36] T. Padmanabhan. Theoretical Astrophysics: Radiative Processes , 2000 .
[37] Roger D. Blandford,et al. On the fate of gas accreting at a low rate on to a black hole , 1998, astro-ph/9809083.
[38] James M. Moran,et al. The Submillimeter Array , 2004, Astronomical Telescopes and Instrumentation.
[39] The Cluster of Galaxies Surrounding Cygnus A , 1997, astro-ph/9708150.
[40] R. Narayan,et al. Advection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991 , 1997, astro-ph/9705237.
[41] F. Honma. Global Structure of Bimodal Accretion Disks around a Black Hole , 1996 .
[42] C. Carilli,et al. Cygnus A , 1996 .
[43] R. Narayan,et al. Advection dominated accretion: Underfed black holes and neutron stars , 1994, astro-ph/9411059.
[44] M. Wright,et al. Mapping Cygnus A at 3 millimeter wavelength with the MIRIAD system , 1993 .
[45] Fulvio Melia,et al. An accreting black hole model for sagittarius A , 1992 .
[46] C. Carilli,et al. Faraday rotation of Cygnus A - magnetic fields in cluster gas , 1987 .
[47] G. Swenson,et al. Interferometry and Synthesis in Radio Astronomy , 1986 .
[48] Richard A. Perley,et al. The Jet and Filaments in Cygnus A , 1984 .
[49] K. Thorne. Disk-Accretion onto a Black Hole. II. Evolution of the Hole , 1974 .