Every Microsecond Counts for this Pulsar!
The optical pulses from a very special pulsar are showing up around 200 microseconds late- today’s authors investigate this very tiny lag to learn why!
The optical pulses from a very special pulsar are showing up around 200 microseconds late- today’s authors investigate this very tiny lag to learn why!
INTEGRAL changed our understanding of X-ray binaries, and taught us so much about our galactic home. Here’s a brief look, in awe and gratitude.
The collision –or even a near-miss– of a neutron star and a main sequence star can possibly explain long-lived, bumpy supernovae and hypervelocity stars.
How do supermassive black holes get to be so supermassive? Today’s authors explore how we might be able to answer that question with the SKA pulsar timing array!
We sit down with Professor Vicky Kaspi and Dr. Paul Scholz, plenary speakers at #AAS240, to hear about their work studying fast radio bursts with the CHIME telescope!
The solar wind is a fascinating thing, but sometimes it can be a big problem. Today’s paper discusses why pulsar astronomers need to worry about it!