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Spiral-like structure in MonR2 as seen with C18O (Trevino-Morales et al., in prep.)
Sandra P. Treviño Morales
Sandra P. Treviño Morales
Astronomer
Postdoctoral researcher working within the PROMISE project at Chalmers University of Technology, Sweden. The main objective of the PROMISE team is to explore how the fundamental physical processes regulate the star formation in the Milky Way.
More specifically, my work within the team consist in the study of the dynamics and fragmentation in filamentary structures from an observational point of view using single-dish facilities (eg., IRAM-30m telescope and the Atacama Pathfinder EXperiment) and radio-interferometers (eg., the Very Large Array and the Atacama Large Millimeter/submillimeter Array).
I am also interested in the study of the chemistry of high-mass star-forming regions.
Top image credit: Column density maps of Orion A derived from Herschel (Stutz & Kainulainen, 2015)
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