What causes clumps in winds from Red Supergiants and Asymptotic Giant Branch stars?

Study the magnetization of water using digital camera and laser beam

Detailing evolved star wind complexity: comparing maser and thermal imaging

Detailed SiO proper motion analysis: slow net expansion and a small correlation with the magnetic field

Multi-epoch Proper Motion Magnetic Field Comparison of SiO Masers around R Cas

Optimal analysis of laser beam propagation through dust storm