Unveiling an important component of Milky Way gas
This paper suggests a new quantity to measure the brightness of gas emission throughout the Milky Way, and determines the regions where most stars are likely to be forming in our Galaxy.
Hypervelocity stars: what are they running from?
Five new hypervelocity stars have been discovered in the outer regions of the Milky Way. In this paper, the authors discuss what these stars are, how they got so far away, and what their distribution implies about the center of our galaxy.
Do we really need a ring?
Understanding the structure of our Milky Way is as difficult as trying to see the forest from the trees. Among the many uncertainties, we don’t know whether the molecular ring is really due to a ring structure or it is simply produced by the spiral arms.
Mealtime for Sgr A*
Remember that tidal disruption event we talked about earlier this year, where a star got just a little too close to a quiescent black hole? Well, here’s our chance to witness something similar, happening in the center of our very own galaxy!
One disk, two disks, red disk, blue disk?
It is written in The Standard Lore of Astronomy – a leather-bound book professors keep under their desks – that stars in the disks of spiral galaxies have a bimodal distribution of scale heights. Today we will be discussing a paper that comes to the conclusion that the notion of a thick disk and a thin disk is actually a poor approximation to the true distribution of disk stars.
Lighting up Simulated Galaxies
For today’s astrobite, we will be discussing some of the highest-resolution simulations of isolated galaxies performed to date. Not only are these simulations high resolution, but they also include prescriptions to model several physical effects that previous galaxy evolution simulations have mostly ignored.