Center for Astrophysics Research and Technologies Seminar Series
Molecular Tracers of Star Formation Feedback in Nearby Galaxies
Presented by Mark Gorski (UNM/NRAO)
The energy and momentum injected into the ISM from stars has a drastic effect on the star formation history of a galaxy. This feedback is responsible for the inefficient collapse of the ISM into stars. By using molecular tracers of feedback, we provide insights into the star forming ecosystem of the galaxies NGC 253, IC 342, NGC 6946, and NGC 2146. We have selected the metastable NH_3 lines as a temperature tracer of the dense molecular ISM, the 22 GHz H_2O maser as an indicator of star formation, and the 36 GHz CH_3OH maser which was previously unexplored in the extragalactic context. We uncover evidence for a uniform two-temperature component distribution of the molecular gas across the central kiloparsec of NGC 253 and IC 342. The temperature does not appear to correlate with feedback effects such as supernovae, PDRs, or shocks. We identify several new water masers associated with star formation across all four galaxies. We also show that extragalactic 36 GHz CH_3OH masers are likely related to large scale weak shocks in the dense molecular ISM. In NGC 253 specifically we test models of galactic outfows driven by a nuclear starburst with sub-arcsecond observations of NH_3(3,3) masers, H_2O masers and CH_3OH masers. We uncover evidence for star formation and entrainment of molecular material in the outflow of NGC 253.
2:00 pm, Thursday, September 14, 2017
Room 190, Physics & Astronomy
Northeast corner of Lomas and Yale, Albuquerque, New Mexico
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