White Paper on East Asian Vision for mm/submm VLBI: Toward Black Hole Astrophysics down to Angular Resolution of 1~R$_{S}$

This White Paper details the intentions and plans of the East Asian Very Long Baseline Interferometry (VLBI) community for pushing the frontiers of millimeter/submillimeter VLBI. To this end, we shall endeavor to actively promote coordinated efforts in the East Asia region. Our goal is to establish firm collaborations among the East Asia VLBI community in partnership with related institutes in North America and Europe and to expand existing global mm/submm VLBI arrays for (a) exploring the vicinity of black holes with an ultimate angular resolution down to 1~R$_{S}$ (Schwarzschild radius) and (b) investigating the dynamics of circumstellar gas in star-forming regions and late-type stars, and circumnuclear gas around active galactic nuclei (AGNs). In the first half of this White Paper, we highlight scientific accomplishments of the East Asia (EA) VLBI community. Various VLBI research results on M87, Sgr A*, blazars, narrow-line Seyfert~1 galaxies, and compact symmetric objects are described, and future visions of our VLBI science are briefly presented. Maser science of star formation, stellar evolution, and physics of accretion disks around AGNs are also discussed. A new vision for conducting multi-transition maser studies using mm/submm VLBI together with the Atacama Large Millimeter/Submillimeter Array (ALMA) is described. In the second half of this White Paper, we describe the EA community's vision for using mm/submm VLBI arrays in the framework or extended version of the Event Horizon Telescope (EHT) and the Global Millimeter VLBI Array (GMVA). The accomplishment of the aforementioned goal will maximize the overall scientific outcomes of mm/submm VLBI in the world.

[1]  William T. Freeman,et al.  Computational Imaging for VLBI Image Reconstruction , 2015, 2016 IEEE Conference on Computer Vision and Pattern Recognition (CVPR).

[2]  Jeff Wagg,et al.  Advancing Astrophysics with the Square Kilometre Array , 2015 .

[3]  Urbana-Champaign,et al.  IMAGING AN EVENT HORIZON: MITIGATION OF SOURCE VARIABILITY OF SAGITTARIUS A* , 2015, 1512.08543.

[4]  M. Kino,et al.  HIGH-SENSITIVITY 86 GHz (3.5 mm) VLBI OBSERVATIONS OF M87: DEEP IMAGING OF THE JET BASE AT A RESOLUTION OF 10 SCHWARZSCHILD RADII , 2015, 1512.03783.

[5]  J. Ott,et al.  The galactic center : Feeding and feedback in a normal galactic nucleus : proceedings of the 303rd symposium of the International Astronomical Union held in Santa Fe, NM, USA, September 30 - October 4, 2013 , 2014 .

[6]  R. Genzel,et al.  The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus , 2014 .

[7]  Alan E. E. Rogers,et al.  PERSISTENT ASYMMETRIC STRUCTURE OF SAGITTARIUS A* ON EVENT HORIZON SCALES , 2016, 1602.05527.

[8]  H. Kobayashi,et al.  Multi-Epoch VERA Observations of Sagittarius A*. I. Images and Structural Variability , 2013, 1308.6657.

[9]  T. Kawashima,et al.  A possible time-delayed brightening of the Sgr A* accretion flow after the pericenter passage of the G2 cloud , 2017, 1702.07903.

[10]  R. Morganti,et al.  Cold gas and the disruptive effect of a young radio jet , 2015, 1511.01613.

[11]  H. Kobayashi,et al.  Fundamental Parameters of the Milky Way Galaxy Based on VLBI Astrometry , 2012, 1211.3843.