T tauri variables can result from this process, which commonly occurs in Bok globules.
A model of this process was generalized by Gerola and Seiden and states that this process propagates through shockwaves generated by stellar winds; that model is SSPSF. An exponent of 1.4 is used to relate the rate of this process to the local gas surface density in the Kennicutt-Schmidt law. This process occurs in regions that have a high infrared excess in a color-color diagram. UV emission into (*) H II regions can propagate this process. T tauri variables can result from this process, which commonly occurs in Bok globules. This process begins after the collapse of a giant molecular cloud, and the result of this process then moves along the H-R diagram. For 10 points, name this process that mainly occurs in stellar nurseries.
A model of this process was generalized by Gerola and Seiden and states that this process propagates through shockwaves generated by stellar winds; that model is SSPSF.
star formation [accept reasonable equivalents like “the creation of a star” or “a star is born”]