2017MNRAS.468L..87C

Properties of the cold interstellar medium of low-metallicity galaxies are not well known due to the faintness and extremely small scale on which emission is expected. We present deep ALMA band 6 (230 GHz) observations of the nearby, low-metallicity (12 + log (O/H) = 7.25) blue compact dwarf galaxy SBS 0335-052 at an unprecedented resolution of 0.2 arcsec (52 pc). The ¹²CO J = 2-1 line is not detected and we report a 3σ upper limit of L_CO(2–1) = 3.6 x 10⁴ K km s^–1 pc². Assuming that molecular gas is converted into stars with a given depletion time, ranging from 0.02 to 2 Gyr, we find lower limits on the CO-to-H2 conversion factor α_CO in the range 10²-10⁴ M_☉ pc^–2 (K km s^–1)^–1. The continuum emission is detected and resolved over the two main super star clusters. Re-analysis of the IR-radio spectral energy distribution suggests that the mm-fluxes are not only free-free emission but are most likely also associated with a cold dust component coincident with the position of the brightest cluster. With standard dust properties, we estimate its mass to be as large as 10⁵ M_☉. Both line and continuum results suggest the presence of a large cold gas reservoir unseen in CO even with ALMA.