Presentation files
13 January, 2019
K. Wada | |
Aalto Susanne (invited) | Feeding and feedback in embedded nuclei - the cold winds of change |
Izumi Takuma (invited) | My collaboration in Kagoshima: to understand the multi-phase obscuring nature of AGNs |
Kawaguchi Toshihiro | Fast and Dense Outflow from Active Galactic Nuclei with High Gas Accretion Rates |
T. Izumi | |
Michiyama Tomonari | ALMA OBSERVATIONS OF HCN AND HCO+ OUTFLOWS IN THE MERGING GALAXY NGC 3256 |
Kishimoto Makoto | Three dimensional structure of AGN gas clouds at 1-100 pc scales |
Nomura Mariko | Radiation Hydrodynamic Simulations of Line-driven Disk Winds: Metallicity Dependence and SMBH Growth |
Baba Shunsuke | AGN torus properties investigated by the CO near-infrared absorption band |
Nakagawa Takao/Onishi Shusuke | Study of molecular-torus structure of active galactic nuclei by observing velocity variation of CO absorption lines |
Imai Hiroshi | A highly-collimated molecular jet from an asymptotic giant branch star ignited 65 years ago |
14 January, 2019
Machida Masahiro (invited) | Protostellar outflows in star formation simulations |
Matsushita Yuko | Outflow driven by the Massive and Intermediate stars : Simulation and Observation |
Hirano Naomi | Outflows from youngest protostars |
Takakuwa Shigehisa | ALMA Observations of Circumbinary Disks in Protostellar Binary Systems |
Lunch Break | |
Masahiro Machida | |
Takasao Shinsuke (invited) | MHD simulations of intermittent outflows from inner protoplanetary disks |
Aso Yusuke | Millimeter sources with and without CO outflows in Serpens Main |
Burns Ross | Observations of jet/outflow rotation using VLBI and ALMA |
Machida Mami | Radio wavelength visualization of spiral galaxies obtained from numerical simulations |
Taniguchi Yoshiaki | Starburst-AGN Connection, Revisited |
Wada Keiichi | Outflow/Fountain in AGNs |
Kudoh Yuki | MHD simulations of tori |
Kawaguchi Takeru | Mass accretion to black holes in late phase of merger process |
Hamamura | Atomic gas structure of AGN in Circinus galaxy |