Avery Bailey, Andrew Youdin, Kaitlin Kratter Astro-ph: arXiv:2603.20373 In this paper, we extend the foundational work of Bondi (1952) to include the effects of radiative feedback in gas-pressure-dominated environments. We construct steady-state spherically symmetric...

Overlap of quiescent K and M dwarfs (red stars) with transiting exoplanet hosts (black dots) in stellar Teff and metallicity space. The range of targets selected for this proposal (blue circled red stars) allows for broad expansion and testing of model atmospheres in...

After an almost 2-year pause due to the pandemic, we restarted our in-person AE Breakfasts. It has been really wonderful to be able to chat face to face about all the cool science!

Protoplanetary disks offer an opportunity to learn about the processes by which planetary systems form and evolve. Images of these young systems also enable us to study, by analogy, the formation of our own Solar System, in which the common orbital plane of the...

The key goal of EOS is to advance our understanding of the formation of habitable planets. As an unusually large and ambitious program, EOS is in a rare position to successfully integrate interdisciplinary knowledge on planet formation – that is, to combine...