The HI-MaNGA survey is an HI (21cm line) follow-up program for the SDSS-IV MaNGA survey. I will describe the HI-MaNGA survey, its progress to date, and future plans. I will then present new results where we combine HI-MaNGA and MaNGA data to investigate how the global HI content of star-forming galaxies relates to the mean properties of their ISM derived from optical emission lines, including integrated equivalent width, metallicity, ionization parameter, and the relative strength of low-ionization lines such as [SII] and [OI]. This analysis allows us to understand if and how the properties of the ISM vary between the most gas-rich galaxies to the most gas-poor, and how such variations may affect their evolution. I will also discuss how gas content relates to the nuclear ionizing source (e.g., Seyfert, LINER, HII regions) and whether we find any evidence that AGN contribute to gas deficiency in the galaxy population.
Online by Zoom
Speaker(s) / Presenter(s):
David V. Stark (Haverford College)