Survey detects 88 new HH objects in Serpens-Aquila Rift and maps five star-forming clouds at 250-700 pc, positioning HH outflows as indicators of active star formation sites.
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Synthetic Herschel observations from simulations yield 8832 filaments hosting 94% of clumps, with power-law mass and length distributions and a density relation qualitatively matching the Hi-GAL survey.
The chapter proposes SKA spectroscopic surveys of the inner and outer Milky Way using OH, CH, radio recombination lines, and H2CO to study molecular cloud formation, ionized gas properties, and CO-dark molecular gas.
citing papers explorer
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Mapping Active Star-Formation in Serpens and the Aquila Rift
Survey detects 88 new HH objects in Serpens-Aquila Rift and maps five star-forming clouds at 250-700 pc, positioning HH outflows as indicators of active star formation sites.
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From filaments to clumps: filament properties with synthetic Herschel observations
Synthetic Herschel observations from simulations yield 8832 filaments hosting 94% of clumps, with power-law mass and length distributions and a density relation qualitatively matching the Hi-GAL survey.
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Spectroscopic surveys with the SKA probing the ionized and molecular Milky Way
The chapter proposes SKA spectroscopic surveys of the inner and outer Milky Way using OH, CH, radio recombination lines, and H2CO to study molecular cloud formation, ionized gas properties, and CO-dark molecular gas.