We investigate 25 H II regions that show bubble morphology in13CO(1–0)and infrared data,to search for quantitative evidence of triggered star formation by proc
This work uses a combination of a variational auto-encoder and generative adversarial network to compare different dark energy models in light of observations,
High-precision proper motions and radial velocities of 1046 stars are used to determine member stars using three-dimensional(3D) kinematics for open cluster NGC
Recent observations have found that chromospheric spicules behave likeAlfvenic fluctuations. Low-frequency Alfven waves are predicted to partially reflectin the