Revisiting GW170817 at milliarcsecond scale: high-precision constraints on jet geometry and Hubble’s constant

Mount Stromlo Observatory in conjunction with the Canberra Astronomical Society invite you to attend our public observing nights of 2054. Come and see the craters of the moon, planets, and beautiful star clusters and nebulae. Object visibility will vary depending on the night.

Fast Radio Bursts

What can we learn from the vast diversity in radio supernovae?

Mount Stromlo Observatory in conjunction with the Canberra Astronomical Society invite you to attend our public observing nights of 2054. Come and see the craters of the moon, planets, and beautiful star clusters and nebulae. Object visibility will vary depending on the night.

In pursuit of realistic star formation histories from SED fitting.

One astronomer's noise is another's signal: Stars, planets and magnetic fields.

Resolving the subgrid physics of galactic winds.

Geodesic Mesh MHD - Modeling Magnetic Massive Stars in 3D; Simulations of a Magnetic O Star