Group Blog

Blog posts by Sera’s group.

Filter posts by category

The best plot in astrophysics

In these last few years many fields in astrophysics have been advancing at an amazing rate. One of the fastest has been the study of the so-called “fast radio bursts” (or FRBs). As the name implies, FRBs are flashes of radio emission that happen extremely fast – down to a few milliseconds. This short duration […]

The best plot in astrophysics Read More »

Warps and twists around black holes

Twisted jets? Warped disks? It’s all possible in black holes! Hi all! Today I will talk a bit about our recent paper on the different types of disks you can have around black holes. As perhaps you would know, in 2019, the Event Horizon Telescope collaboration (EHTC) released the first-ever photos of the inner regions

Warps and twists around black holes Read More »

What cooling can do for Sagittarius A*

Making an assumption is inevitable and reasonable in many research projects since it is practically impossible to handle all physics we know in a single study; even if it is feasible, it would rather squander resources, which are given to us. However, it is always required to evaluate carefully whether the assumptions are applicable for

What cooling can do for Sagittarius A* Read More »

Things need to change

This is going to be a hard post for me to write, and for everyone to read. It will not discuss science, because today I want to talk about something that I think is far more important.TW: sexual assault discussion below. My main hobby is PC gaming, and many of my favorite games (Starcraft 1

Things need to change Read More »

The runner’s trails: the characteristic features of fast-moving X-ray Binaries or Bow-shock Pulsars

In today’s post, I will talk about a subset of compact objects (neutron stars or stellar mass black holes), which run with very high spatial velocity through the interstellar medium. Those runners, in general, imprint characteristic signatures on their way: trails and bubbles. For the case of static objects (i.e., no proper motion), which the

The runner’s trails: the characteristic features of fast-moving X-ray Binaries or Bow-shock Pulsars Read More »

Scroll to Top