Mark Siebert
My research focuses on the mass-loss of evolved stars. I primarily use molecular line observations from today's radio and submillimeter telescopes to unravel the dynamics, evolution, and chemistry of winds surrounding RSG, AGB, and post-AGB stars. I also have experience studying complex carbon chemistry in pre-stellar clouds.
Showing 3 publications
Molecular Distributions and Abundances in the Binary-shaped Outflow of V Hya
Stephenson 2 DFK 52: Discovery of an exotic red supergiant in the massive stellar cluster RSGC2
Detection of interstellar 1-cyanopyrene: A four-ring polycyclic aromatic hydrocarbon
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