is mass distributed between neutral gas phases? 21-SPONGE There is a significant amount of thermally unstable HI in the local ISM 52% 20% 28% WNM UNM CNM Murray et al. 2018b
is mass distributed between neutral gas phases? “Total gas” = HI + CO Optically-thick HI cannot solely account for ``dark” gas ``Dark” correction assuming excess dust = HI (Fukui et al. 2015) ``Dark” correction measured by 21cm absorption Murray, Peek et al. 2018
Kim 2020 slope More cold, optically-thick HI Diffuse HI HI dominates 1<N(HI)<4e20 cm-2 Even for diffuse, high-latitude gas, the correlation between E(B-V) and N(HI) depends on amount of cold HI
Kim 2020 slope More cold, optically-thick HI Diffuse HI HI dominates 1<N(HI)<4e20 cm-2 Even for diffuse, high-latitude gas, the correlation between E(B-V) and N(HI) depends on amount of cold HI
gas the Small Magellanic Cloud? Di Teodoro et al. 2019 Motions of young stars embedded in the ISM are more complicated than rotation alone Murray, Peek, Di Teodoro et al. 2019
github.com/BEAST-Fitting/beast PI Murray, Gordon, McQuinn, Yanchulova Merica-Jones, Lindberg, Williams +ISM@ST 500-orbit Hubble Space Telescope parallel UV-NIR imaging survey with WFC3 Dissecting the Magellanic Clouds with Scylla
github.com/BEAST-Fitting/beast PI Murray, Gordon, McQuinn, Yanchulova Merica-Jones, Lindberg, Williams +ISM@ST 500-orbit Hubble Space Telescope parallel UV-NIR imaging survey with WFC3 Dissecting the Magellanic Clouds with Scylla
github.com/BEAST-Fitting/beast PI Murray, Gordon, McQuinn, Yanchulova Merica-Jones, Lindberg, Williams +ISM@ST 500-orbit Hubble Space Telescope parallel UV-NIR imaging survey with WFC3 Dissecting the Magellanic Clouds with Scylla
github.com/BEAST-Fitting/beast PI Murray, Gordon, McQuinn, Yanchulova Merica-Jones, Lindberg, Williams +ISM@ST 500-orbit Hubble Space Telescope parallel UV-NIR imaging survey with WFC3 Dissecting the Magellanic Clouds with Scylla CO (1-0) contours
github.com/BEAST-Fitting/beast PI Murray, Gordon, McQuinn, Yanchulova Merica-Jones, Lindberg, Williams +ISM@ST 500-orbit Hubble Space Telescope parallel UV-NIR imaging survey with WFC3 Dissecting the Magellanic Clouds with Scylla LMC SMC 58 60 62 64 66 AV