Review Article: Protoplanetary Disks and Their Evolution

Review Article: Protoplanetary Disks and Their Evolution

In a new review article, Jonathan Williams and Lucas Cieza at the Institute for Astronomy (IfA) describe the life-story of protoplanetary disks from formation from collapsing molecular clouds to the end-state of a planetary system. Infrared telescopes like Spitzer and sub-millimeter radio telescopes like the the James Clerk Maxwell Telescope, the Submillimeter Array (SMA), and the Combined Array for Research in Millimeter Astronomy (CARMA) have greatly revolutionized the study of protoplanetary disks because they can probe the emission at the longer wavelengths where the disk emission is strongest.

Dense, Ionized Hydrogen near the Galactic Center of the Milky Way

Dense, Ionized Hydrogen near the Galactic Center of the Milky Way

It turns out that there is a lot more to the universe than just stars, planets, and galaxies. Much of the “empty space” between these objects is actually host to interesting astrophysical processes, such as star-formation in molecular clouds. Hot, young stars can emit strong radiation that will ionize the surrounding hydrogen gas. Astronomers call these dense regions of ionized hydrogen HII regions.

The Databases of Astronomy: Organizing the Knowledge of the Field

The Databases of Astronomy: Organizing the Knowledge of the Field

Astronomy is a field that has written records that date far back in history, much of it published in journals, books, and letters. However, only in the later part of the 20th century did the vast tomes of astronomical information meet the internet. Online tools now make it possible to access practically every paper or article ever published and visualize vast amounts of data from telescope archives. This post (to be updated incrementally in the future) will serve as an overview to some of the organizational tools of astronomy that astrobites authors have come to use and love.