Astro 2020 White Paper: Understanding Accretion Outbursts in Massive Protostars through Maser Imaging Thematic Area: Star and Planet Formation Todd Hunter 1 (520 Edgemont Rd, Charlottesville, VA, thunter@nrao.edu), Co-authors: Anna Bartkiewicz 2 , Walter Brisken 1 , Crystal L. Brogan 1 , Ross Burns 3 , James O. Chibueze 4 , Claudia J. Cyganowski 5 , Tomoya Hirota 3 , Gordon MacLeod 6,7 , Alberto Sanna 8 and Jos´ e-Mar´ ıa Torrelles 9 1 National Radio Astronomy Observatory (NRAO) 2 Nicolaus Copernicus University, Torun, Poland 3 National Astronomical Observatory of Japan (NAOJ) 4 Centre for Space Research, North-West University 5 School of Physics and Astronomy, University of St. Andrews 6 Hartebeesthoek Radio Astronomy Observatory (HartRAO) 7 University of Western Ontario 8 Max-Planck-Institut f¨ ur Radioastronomie (MPIfR) 9 Institut de Ci` encies de l’Espai (CSIC) February 22, 2019 Abstract The bright maser emission produced by several molecular species at centimeter to long millimeter wavelengths provides an essential tool for understanding the process of massive star formation. Unimpeded by the high dust optical depths that affect shorter wavelength observations, the high brightness temperature of these emission lines offers a way to resolve accretion and outflow motions down to scales below ∼1 au in deeply embedded Galactic star-forming regions at kiloparsec distances. The recent identification of extraordinary accretion outbursts in two high-mass protostars, both of which were heralded by maser flares, has rapidly impacted the traditional view of mas- sive protostellar evolution, leading to new hydrodynamic simulations that can produce such episodic outbursts. In order to understand how these massive protostars evolve in response to such events, larger, more sensitive ground-based centimeter wavelength interferometers are needed that can simultaneously image multiple maser species in the molecular gas along with faint continuum from the central ionized gas. Fiducial obser- vations of a large sample of massive protostars will be essential in order to pinpoint the progenitors of future accretion outbursts, and to quantify the outburst-induced changes in their protostellar photospheres and outflow and accretion structures. Knowledge gained from these studies will have broader impact on the general topic of accretion onto massive objects. arXiv:1903.09306v1 [astro-ph.SR] 21 Mar 2019