Masquerade! Dwarf Nova Faces on Parade
ISO classical novae! We aren’t seeing as many classical novae as we expect. Read on to find out if they’re masquerading as dwarf novae!
ISO classical novae! We aren’t seeing as many classical novae as we expect. Read on to find out if they’re masquerading as dwarf novae!
Today’s paper looks at GD 424, a very hungry white dwarf that is accreting planets!
Astronomers discover a planetary fragment that survived the destruction of its host star – offering insights into the future of planetary systems like our own.
Imagine going from having data on 250 white dwarfs to almost 14,000 overnight… Thanks to the latest Gaia data release, this dream became reality, allowing astronomers to look for patterns in the local white dwarf population for the very first time.
We thought we knew how quickly the white dwarf pulsar in AR Scorpii was spinning down, but a new study tells us we can’t know for sure.
To unlock the secrets of the (local) universe, Adam Riess observes the brightness of supernovae and Cepheid variables to measure the distance to galaxies far, far away. Read more about his research before his plenary talk at #AAS231 on Tuesday.