Primordial Origin of Magnetic Fields in the Galaxy & Galaxies - Tight Link between GC and Cosmic B –  Y. Sofue1, M. Machida2, T. Kudoh3 (1. Kagoshima.

Slides:



Advertisements
Similar presentations
(2) Profile of the Non-Thermal Filaments of SNRs =>High Energy Particle Acceleration =>High Energy Particle Acceleration In all the SNRs & GC Non Thermal.
Advertisements

Hi-GAL PI: Sergio Molinari (Rome) + Hi-GAL team … (~150 researchers)
Toyoaki Suzuki (ISAS/JAXA) Hidehiro Kaneda (Nagoya Univ.) Takashi Onaka (Tokyo Univ.)
NGC 5128 – Centaurus A Dante Minniti ESO Vitacura Nov 2005.
Dark Matter in Dwarf Galaxies
May 17, 2010MFPO 2010, Krakow1 Dwarf galaxies and the Magnetisation of the IGM Uli Klein ?
Study of Cosmic Magnetic Fields with Square Kilometer Array Keitaro Takahashi Nagoya University workshop 2010.
Jets from Active Galactic Nuclei: Observations and Models
渦状銀河における GMC の進化と星形 成 Evolution of GMCs and star formation in spiral galaxies Nario Kuno Nobeyama Radio Observatory 1.NRO M33 All-Disk Survey of Giant.
Contamination of the CMB Planck data by galactic polarized emissions L. Fauvet, J.F. Macίas-Pérez.
Katarzyna Otmianowska-Mazur (OA UJ Kraków)‏ Grzegorz Kowal (Uniw. Sao Paulo, Brazylia/OA UJ Kraków)‏ Katarzyna Kulpa-Dybeł (OA UJ Kraków) Hubert Siejkowski,
Particles and Fields in Lobes of Radio Galaxies Naoki Isobe (NASDA, MAXI Mission) Makoto Tashiro (Saitama Univ.) Kazuo Makishima (Univ. of Tokyo) Hidehiro.
T.G.Arshakian MPI für Radioastronomie (Bonn) Exploring the weak magnetic fields with LOFAR.
Galactic Magnetic Field Research with LOFAR Wolfgang Reich Max-Planck-Institut für Radioastronomie Bonn, Germany.
Krakow 2010 Galactic magnetic fields: MRI or SN-driven dynamo? Detlef Elstner Oliver Gressel Natali Dziourkevich Alfio Bonanno Günther Rüdiger.
Radio continuum, CO, and thermal infrared emission in nearby star-forming galaxies Tony Wong CSIRO Australia Telescope & University of New South Wales.
Y. Sofue I. Correlation among RM, HI, FF, & Synch. Emissions.
Our Galaxy The Milky Way. The Milky Way Almost everything we see in the night sky belongs to the Milky Way We see most of the Milky Way as a faint band.
Dynamics of Multi-Phase Interstellar Medium Shu-ichiro Inutsuka (Nagoya Univ) Thanks to Hiroshi Koyama (Univ. Maryland) Tsuyoshi Inoue (Kyoto Univ.) Patrick.
Molecular absorption in Cen A on VLBI scales Huib Jan van Langevelde, JIVE Ylva Pihlström, NRAO Tony Beasley, CARMA.
Magnetic fields in our Galaxy JinLin Han National Astronomical Observatories Chinese Academy of Sciences Beijing, China Thanks for cooperation.
Subgrid models of active galactic nuclei in clusters of galaxies Paul Matthew Sutter Paul M. Ricker Univ. of Illinois at Urbana-Champaign Frontiers in.
Cosmic magnetism ( KSP of the SKA) understand the origin and evolution of magnetism in the Galaxy, extragalactic objects, clusters and inter-galactic/-cluster.
Physics 231: Section 6 Galaxies 1Phys 231, Topic 6: Galaxies.
Three-dimensional MHD Simulations of Jets from Accretion Disks Hiromitsu Kigure & Kazunari Shibata ApJ in press (astro-ph/ ) Magnetohydrodynamic.
The Galactic Center at Low Radio Frequencies Namir Kassim (NRL) Crystal Brogan (IfA) J. Lazio (NRL), Ted LaRosa (Kennesaw State), M. Nord (NRL/UNM), W.
Structure Function of Rotation Measure toward High Galactic Latitudes Takuya Akahori 1,2 1 Radio Astronomy Division, KASI 2 Research Fellow for Young Scientist,
Cosmic Magnetic Fields: Helicity Injection by Supermassive Black Holes, Galaxies and Laboratory Experiments Hui Li 李暉 Los Alamos National Laboratory and.
銀河系は爆発したか ? 孤軍奮闘の30年論争 祖父江義明 200 銀河ゼミ. 太陽は爆発する.
Magnetic fields in the Galaxy via Faraday effect: Future prospects with ASKAP and the SKA Lisa Harvey-Smith Collaborators: Bryan CSIRO SKA Project ScientistGaensler.
Hajime Takami Institute for the Physics and Mathematics of the Universe, the University of Tokyo High Energy Astrophysics KEK, Tsukuba, Nov. 11,
Cosmic magnetism ( KSP of the SKA)‏ understand the origin and evolution of magnetism in the Galaxy, extragalactic objects, clusters and inter-galactic/-cluster.
Kashi1 Radio continuum observations of the Sombrero galaxy NGC4594 (M104) and other edge-on spirals Marita Krause MPIfR, Bonn Michael Dumke ESO,
H 3 + Toward and Within the Galactic Center Tom Geballe, Gemini Observatory With thanks to Takeshi Oka, Ben McCall, Miwa Goto, Tomonori Usuda.
Galaxies with Active Nuclei Chapter 14:. Active Galaxies Galaxies with extremely violent energy release in their nuclei (pl. of nucleus).  “active galactic.
Sawtooth-like Oscillations of Black Hole Accretion Disks Ryoji Matsumoto (Chiba Univ.) Mami Machida (NAOJ)
Jet Interactions with the Hot Atmospheres of Clusters & Galaxies B.R. McNamara University of Waterloo Girdwood, Alaska May 23, 2007 L. Birzan, P.E.J. Nulsen,
1 Stellar molecular jets trace by maser emission Hiroshi Imai (Kagoshima University) IAU Symposium 242: 14 March 2007, Alice Springs, Australia.
Searching for the Synchrotron Cosmic Web with the Murchison Widefield Array Bryan Gaensler Centre for All-sky Astrophysics / The University of Sydney Natasha.
Fermi LAT Observations of Galactic and Extragalactic Diffuse Emission Jean-Marc Casandjian, on behalf of the Fermi LAT collaboration 7 questions addressed.
Seeding the ICM: Primordial or Astrophysical? Jungyeon Cho Chungnam National University, Korea Cho & Yoo (2012; ApJ) Cho (2013; PRD) Cho (2014, ApJ) Origin.
Simulations for the nearby Seyfert 2 galaxy NGC 4945 Lien-Hsuan Lin 1,2, Chi Yuan 2, C.C. D. Yen 3, and S. Muller 2 1 Department of Physics, National Taiwan.
Studying ISM and star formation in M33 with ALMA Sachiko Onodera & NRO MAGiC Team: (M33 All-disk Survey of Giant Molecular Clouds) N. Kuno 1, T. Tosaki.
Molecular gas in cooling flows Interplay with AGN and starbursts
Galaxies Chapter 23.
Theoretical Astrophysics Group
Molecular Gas Distribution of our Galaxy: NANTEN Galactic Plane Survey
LARGE PICTURE OF THE GALACTIC CENTER STUDIED BY H3+:
Galactic Magnetism with SKA: Primordial Origin of BSS, ASS, Ring &Vertical Fields Y. Sofue1,2, M. Machida3, T. Kudoh3, H. Nakanishi1 (1. Kagoshima U.,
Morphology of the Galactic center from the H3+ spectrum:
Why Warps ?… Accretion, Recycling, Stimulation ?
Dense gas history of the Universe  Tracing the fuel for galaxy formation over cosmic time SF Law SFR Millennium Simulations, Obreschkow & Rawlings 2009;
The origin of gas in debris disks
Overall distribution of gas and light in the Galaxy
Active Versus Normal Galaxies
My recent research interest focuses on the equatorial upwelling and the associated cold tongue sea surface temperature (SST) evolution. My study (Wang.
Extragalactic Background Fluctuation from the Numerical Galaxies
Dark matter and anomalous gas in the spiral galaxy NGC 4559
3D Galactic Shock Wave at W43 in the 4-kpc Arm
Millimeter Megamasers and AGN Feedback
Galactic Center Rotation Curve and Mass Yoshiaki Sofue (Meisei Uni
「Cosmic-rays and diffused gamma-rays」
Energy spectra of small scale dynamos with large Reynolds numbers
Our Galactic Center and its Environmemt K. Koyama A. Senda
The Local Dark Matter Density Yoshiaki Sofue (U-Tokyo & Meisei-U)
Primordial Origin of Magnetic Fields in the Galaxy & Galaxies - Tight Link between GC and Cosmic B -  Y. Sofue1, M. Machida2, T. Kudoh3 (1. Kagoshima.
VNGS science highlight: PDR models of M51
(spectroscopically confirmed)
SKADS Polarization Simulations The MPIfR team (Milky Way & star-forming galaxies): Tigran Arshakian, Rainer Beck, Marita Krause, Wolfgang Reich, XiaoHui.
Internal Extinction in SDSS Galaxies
Presentation transcript:

Primordial Origin of Magnetic Fields in the Galaxy & Galaxies - Tight Link between GC and Cosmic B –  Y. Sofue1, M. Machida2, T. Kudoh3 (1. Kagoshima U. &. U .Tokyo, 2.Nagoya Univ. 3. NAOJ)

Vertical B in GC vs Spiral/Ring/Loop Fields in the Disks M51, M81, M33, Spiral/Ring + GC V field NGC 2903, Helical jets NGC 253 Helical B, Loops, Jets, Spicules

Galactic Shells, Loops, Jets, Helix 1970’s~ HI, Dust, cold gas HI shells, worms (Heiles 2004) G40 1-kpc HI jets (Sofue 2004)

300 MHz Threads

⊥Galactic Center Vertical B NRO 45m, Bonn 100m Tsuboi et al, 1986, Sofue,et al. 1987

Galactic Center Vertical B: Helical B, Jets, Loops

NGC253 Jets, Loops

NGC 253, NGC 2903 Central Helical Jets

Loop: N2903

M51, M81, M31, Spiral/Ring ⊥ GC V field

2. Primordial origin for S, A, R, & V fields S (BSS) V A (ASS) R (Ring) R amplification SV SRV GC-V field linked to Cosmic B References: (a) Sofue et al. 1986 ARAA 24, 459; (b) 2009 PASJ submitted

SV GC-V field linked to Cosmic B

3. MHD Simulation i=0, 45, 89, 90 deg, 10 kpc disk  ρ&B2 2009 PASJ submitted