446 citations · 2k across the 55 of their papers we have counts for
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A VLA search for compact radio sources in the explosive molecular outflows DR 21 and G5.89
Vanessa Yanza, Sergio A. Dzib, Aina Palau +3
We present high-angular-resolution () VLA Ku-band (12--18 GHz) observations of two explosive molecular outflows (EMOs), DR 21 and G5.89, in a search for runaway s…
The past, present and future of observations of externally irradiated disks
Planet formation environments collaboration, Megan Allen, Rossella Anania +51
Recent years have seen a surge of interest in the community studying the effect of ultraviolet radiation environment, predominantly set by OB stars, on protoplanetary disc evolutio…
Bow shocks, bow waves, and dust waves. IV. Shell shape statistics
William J. Henney, Jorge A. Tarango-Yong, Luis Ángel Gutiérrez-Soto +1
Stellar bow shocks result from relative motions between stars and their environment. The interaction of the stellar wind and radiation with gas and dust in the interstellar medium…
Bow shocks, bow waves, and dust waves. III. Diagnostics
William J. Henney, S. J. Arthur
Stellar bow shocks, bow waves, and dust waves all result from the action of a star's wind and radiation pressure on a stream of dusty plasma that flows past it. The dust in these b…
Bow shocks, bow waves, and dust waves. II. Beyond the rip point
William J. Henney, S. J. Arthur
Dust waves are a result of gas-grain decoupling in a stream of dusty plasma that flows past a luminous star. The radiation field is sufficiently strong to overcome the collisional…
Bow shocks, bow waves, and dust waves. I. Strong coupling limit
William J. Henney, S. J. Arthur
Dust waves and bow waves result from the action of a star's radiation pressure on a stream of dusty plasma that flows past it. They are an alternative mechanism to hydrodynamic bow…