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Experimental and Theoretical Investigation of the Reaction of C2H with Formaldehyde (CH2O) at Very Low Temperatures and Application to Astrochemical Models. [PDF]
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Metal Abundances in the Hot ISM of Elliptical Galaxies
2011X-ray spectroscopy provides a powerful tool to measure various elemental abundances in the hot ISM and the measured abundances in turn can be compared with galaxy chemical evolution models to constrain important astrophysical quantities and to help our understanding of the formation and evolution of elliptical galaxies and their ISM. In this chapter, I
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Go beyond radial gradient: azimuthal variations of ISM abundance in 3D
Proceedings of the International Astronomical Union, 2018AbstractUsing 3D spectroscopy data from the TYPHOON Project (PI: B. Madore), I show convincing observational evidence that the ISM oxygen abundance traced by HII regions presents systematic azimuthal variations in NGC 1365 and NGC 2997. I discuss a possible physical origin and on-going efforts to explore the prevalence and cause of such variations.
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ABUNDANCE RATIOS AND GALACTIC CHEMICAL EVOLUTION
Annual Review of Astronomy and Astrophysics, 1997Andrew McWilliam
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New Light on Stellar Abundance Analyses: Departures from LTE and Homogeneity
Annual Review of Astronomy and Astrophysics, 2005Martin Asplund
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Abundances of the elements in the solar system
Space Science Reviews, 1973A G W Cameron, A G W Cameron
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New calibrations for abundance determinations in H ii regions
Monthly Notices of the Royal Astronomical Society, 2016Eva Grebel, L S Pilyugin
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