Southampton 1 The Disc-Jet connection in LINERS: (and Seyferts..) AMI and X-ray monitoring of M81* Ian M c Hardy, University of Southampton Guy Pooley,

Slides:



Advertisements
Similar presentations
1 VO Theory Use Cases – Intermediate Scale David De Young Project Scientist US NVO IVOA Theory Interest Group S. Lorenzo del Escorial - 10/05.
Advertisements

Authors: A.Bliss, D.M.Worrall, M.Birkinshaw (Bristol), H.Tananbaum, S.Murray (Harvard-Smithsonian C.f.A.) Fig.1: Combined IVU band image, J circled.
The ubiquitous UV murmurs of sleeping supermassive BHs Dani Maoz With: Neil Nagar, Heino Falcke, Andrew Wilson.
X-ray spectral variability of seven LINER nuclei with XMM-Newton and Chandra data Author: Hernandez-Garcia, L; Gonzalez-Martin, O; Marquez, I; Masegosa.
Disk corona in AGN: what do we expect? Bifang Liu Yunnan Observatory, CAS The disk corona evaporation model The model for X-ray binaries Similarities between.
1)Disks and high-mass star formation: existence and implications 2)The case of G : characteristics 3)Velocity field in G31.41: rotation or expansion?
Longterm X-ray observation of Blazars with MAXI Naoki Isobe (Kyoto University; & MAXI
Gabriele Giovannini Dipartimento di Astronomia, Bologna University Istituto di Radioastronomia - INAF EVN observations of M87 as follow-up on a recent.
Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen Liske European Southern Observatory Frank Briggs Australian.
5GHz, VLA image of Cyg A by R. Perley Cosmological growth of SMBH: the kinetic luminosity function of AGN IAU Symposium 238Prague22/08/2006 IAU Symposium.
Radio Loud AGN in 2XMMi Multi-wavelength view A. Labiano (ESAC-ESA), M. Guainazzi (ESAC-ESA), S. Bianchi (Rome-3), G. Miniutti (CAB-INTA)
The disk-jet link: X-ray and radio monitoring of PKS Mario Gliozzi (GMU) I. Papadakis (Crete) W. Brinkmann (MPE) L. Kedziora-Chudczer (Sidney)
Ray Norris, Jamie Stevens, et al. Deep CABB observations of ECDFS ( Extended Chandra Deep Field South )
Low-Luminosity AGN Heino Falcke Max-Planck Institut für Radioastronomie, Bonn Neil Nagar, Andrew S. Wilson Sera Markoff, Feng Yuan.
Portrait of a Forming Massive Protocluster: NGC6334 I(N) Todd Hunter (NRAO/North American ALMA Science Center) Collaborators: Crystal Brogan (NRAO) Ken.
SZE in WMAP Data Jose M. Diego & Bruce Partridge 2010, MNRAS, 402, 1179 La Thuile, March 2012.
A rough guide to radio astronomy and its use in lensing studies Simple stuff other lecturers may assume you know (and probably do)
Swift/BAT Hard X-ray Survey Preliminary results in Markwardt et al ' energy coded color.
Naoki Isobe, Yoshihiro Ueda (Kyoto University) Kousuke Sugimori, Nobuyuki Kawai (Tokyo Tech.) Hitishi Negoro (Nihon Univ.) Mutsumi Sugizaki, Masaru Matsuoka.
WALTER MAX-MOERBECK OWENS VALLEY RADIO OBSERVATORY CALIFORNIA INSTITUTE OF TECHNOLOGY The OVRO 40m 15 GHz Monitoring Program.
School of something FACULTY OF OTHER School of Physics & Astronomy FACULTY OF MATHEMATICS & PHYSICAL SCIENCES AMI and Massive Star Formation Melvin Hoare.
Engine-Driven Supernovae Alicia M. Soderberg Caltech Astronomy Dept. Zwicky Supernova Workshop January
Two years of blazar monitoring with the OVRO 40m telescope at 15GHz in support of the Fermi GST Vasiliki Pavlidou (Caltech) on behalf of the OVRO 40m team.
1 Disk-Jet Connection in the Radio Galaxies 3C 120 and 3C 111 Ritaban Chatterjee NERQUAM 2010, May 18th, 2010.
Multi-wavelength AGN spectra and modeling Paolo Giommi ASI.
Molecular absorption in Cen A on VLBI scales Huib Jan van Langevelde, JIVE Ylva Pihlström, NRAO Tony Beasley, CARMA.
1 Arecibo Synergy with GLAST (and other gamma-ray telescopes) Frontiers of Astronomy with the World’s Largest Radio Telescope 12 September 2007 Dave Thompson.
1 The Fundamental Plane Relationship of Astrophysical Black Holes Ran Wang Supervisor: Xuebing Wu Peking University Ran Wang Supervisor: Xuebing Wu Peking.
An Exceptional Radio Flare in Markarian 421 Joseph L. Richards, Talvikki Hovatta, Matthew L. Lister, Anthony C. S. Readhead, Walter Max-Moerbeck, Tuomas.
… and AGN Marcello Giroletti Dipartimento di Astronomia, UniBO Istituto di Radioastronomia, INAF.
Optical Observations of J : An LMXB in Transition Paul A. Mason New Mexico State University Emmanuel Gonzalez University of Texas at El Paso Edward.
Statistical analysis of model-fitted inner-jets of the MOJAVE blazars Xiang Liu, Ligong Mi, et al. Xinjiang Astronomical Observatory (Former Urumqi Observatory),
The luminous X-ray hotspot in 4C 74.26: jet dynamics at work Mary Erlund Institute of Astronomy, Cambridge, UK A.C. Fabian, K.M. Blundell, C. Moss and.
Imaging Compact Supermassive Binary Black Holes with VLBI G. B. Taylor (UNM), C. Rodriguez (UNM), R. T. Zavala (USNO) A. B. Peck (CfA), L. K. Pollack (UCSC),
Light Curves These light curves were taken by the Swift Gamma-Ray Burst Explorer & Rossi X-Ray Timing Explorer Each graph plots the counts of x-rays with.
Multiwaveband Opportunities to Study AGN (Mostly Blazars) Detected by Fermi Alan Marscher Boston University, Incoming Chair of Fermi Users Group Research.
The Environments of Galaxies: from Kiloparsecs to Megaparsecs August 2004 Cool Cores in Galaxy Groups Ewan O’Sullivan Harvard-Smithsonian Center for Astrophysics.
RADIO OBSERVATIONS IN VVDS FIELD : PAST - PRESENT - FUTURE P.Ciliegi(OABo), Marco Bondi (IRA) G. Zamorani(OABo), S. Bardelli (OABo) + VVDS-VLA collaboration.
THE HST VIEW OF LINERS AND OTHER LOCAL AGN MARCO CHIABERGE CNR - Istituto di Radioastronomia - Bologna Alessandro Capetti (INAF-OATo) Duccio Macchetto.
A synthetic view of AGN evolution and Supermassive black holes growth Leiden 25/11/2009 5GHz, VLA image of Cyg A by R. Perley Andrea Merloni Excellence.
Abstract LS 5039 and LS I are exceptionally rare examples of HMXBs with MeV-TeV emission, making them two of only four known "  -ray binaries".
Gabriele Giovannini Dipartimento di Astronomia, Bologna University Istituto di Radioastronomia - INAF Low Luminosity Radio Loud AGNs In collaboration with.
I.Introduction  Recent evidence from Fermi and the VLBA has revealed a strong connection between ɣ -ray emission in AGNs and their parsec-scale radio.
Long-term X-ray and optical variability of radio-quiet AGN Phil Uttley, University of Southampton with: Ian McHardy, University of Southampton Iossif Papadakis,
X-ray / Radio Correlation for Sub-Eddington Black Holes Heino Falcke ASTRON, Dwingeloo University of Nijmegen, with Elmar Körding, Sera Markoff, Geoff.
Blazars: VLBA and GLAST Glenn Piner Whittier College.
Tobias Jogler Max-Planck Institute for Physics Taup 2007 MAGIC Observations of the HMXB LS I in VHE gamma rays Tobias Jogler on behalf of the MAGIC.
Accretion flows onto black holes
MAGIC Recent AGN Observations. The MAGIC Telescopes Located at La Palma, altitude 2 200m First telescope in operation since 2004 Stereoscopic system in.
A Catalog of Candidate High-redshift Blazars for GLAST
Answers from the Working Group on AGN and jets G. Moellenbrock, J. Romney, H. Schmitt, V. Altunin, J. Anderson, K. Kellermann, D. Jones, J. Machalski,
Shih-Ping Lai 賴詩萍 (National Tsing-Hua University, Taiwan) 清華大學, 台灣.
The Character of High Energy Emission From The Galactic Binary LS Andy Smith Smithsonian Astrophysical Observatory (for the VERITAS collaboration)
Analysis of strong outbursts in selected blazars. Pyatunina T.B., Kudryavtseva N.A., Gabuzda D.C., Jorstad S.G., Aller M.F., Aller H.D., Terasranta H.
A new model for emission from Microquasar jets Based on works by Asaf Pe’er (STScI) In collaboration with Piergiorgio Casella (Southampton) March 2010.
The History of Active Galaxies A.Barger, P. Capak, L. Cowie, RFM, A. Steffen, and Y. Yang Active Galaxies (AKA quasars, Seyfert galaxies etc) are radiating.
Fast Infrared Flickering from GRS The Spirit of Stephen Eikenberry (University of Florida) As Channeled by David Rothstein (Cornell University)
New evidence for extreme particle acceleration in Microquasars Edoardo Striani on behalf of the AGILE Team.
Brigthest Cluster Galaxies Unique class of objects  most luminous  most massive  extended source  some BCG shows multiple nuclei → galaxy merger →
J. L. Higdon, S. J. U. Higdon, D. Weedman, J. Houck (Cornell) B. T. Soifer (Caltech), B. Jannuzi, A. Dey, M. Brown (NOAO) E. Le Floc’h, & M. Rieke (Arizona)
The Dichotomy of Seyfert Galaxies at Hardest X-rays
The central few parsec region of AGN in the IR
The black hole fundamental plane: revisit with a larger sample of radio and X-ray emitting broad line AGNs Zhao-Yu Li Astronomy Department, Peking University.
Evidence for an Intermediate Mass Black Hole in NGC 5408 X-1
From radio to gamma-rays: 3C 273 reveals its multi-component structure
Cygnus X-1 is a Black Hole Binary
A.Malizia, L. Bassani , M. Molina
Group Nov. 01, USTC 4/18/2019 Group Nov. 01, USTC AGN-dominated SFG-dominated.
ZHANG Yue HXMT Collaboration
Modeling Sgr A* Flares: Nonthermal Processes in an Outflow
Presentation transcript:

Southampton 1 The Disc-Jet connection in LINERS: (and Seyferts..) AMI and X-ray monitoring of M81* Ian M c Hardy, University of Southampton Guy Pooley, MRAO

Southampton 2 Do LINERS show same strong radio/X-ray correlation as hard state X-ray Binaries?

Southampton 3 Previous observations: LINER NGC7213 Bell et al, 2011 S ~   MJD-50000

Southampton 4 NGC7213 (Bell et al)

Southampton 5 M81 X-ray and 15GHz lightcurves Swift keV (Richards, Readhead)

Southampton 6 M81 X-ray and 15GHz Cross-correlation

Southampton 7 M81 X-ray and 15GHz lightcurves

Southampton 8 M81 X-ray and 15GHz F R ~F X 0.7 From Falcke et al 2004 cf Merloni et al 2003 observed Mass-scaling following Falcke jet model

Southampton 9 Disc-Jet Connection in `radio quiet’ AGN: Seyferts Jones et al, 2011 Peak flux ~0.5mJy in A-array NGC4051: VLA A and B array 8GHz observations

Southampton 10 NGC4051 VLA A array observations

Southampton 11 NGC4051 Radio vs. X-ray - all arrays No strong evidence for large amplitude radio variability

Southampton 12 Seyfert NGC5548 – brighter in radio than NGC4051 Wrobel no parallel X-ray observations

Southampton Disc-Jet connection in Seyferts 13 AMI 15GHz map of NGC5548 Core easily distinguished

Southampton 14 Conclusion AMI has an excellent capability for monitoring the radio cores in LINERS and `radio-quiet’ AGN. Strong radio/X-ray correlation seen in LINER M81* greatly strengthening the link to hard state XRBs. Radio/X-ray link is unknown in Seyferts (radio quiet AGN) but could easily be studied with AMI.