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Stored in the archives: Uncovering the CN/CO intensity ratio with ALMA in nearby U/LIRGs
Blake Ledger, Toshiki Saito, Daisuke Iono +1
We present an archival Atacama Large Millimeter/submillimeter Array (ALMA) study of the CN N = 1 - 0 / CO J = 1 - 0 intensity ratio in nearby (z < 0.05) Ultra Luminous and Luminous…
J0107a: A Barred Spiral Dusty Star-forming Galaxy at
Shuo Huang, Ryohei Kawabe, Kotaro Kohno +7
Dusty Star-Forming Galaxies (DSFGs) are amongst the most massive and active star-forming galaxies during the cosmic noon. Theoretical studies have proposed various formation mechan…
On the origin of cosmic-ray ionisation in star-forming regions
Marco Padovani
A field with particularly exciting results over the past few years is the study of the interaction of cosmic rays with interstellar matter. For star formation to take place, gas an…
The LMC+ SOFIA Legacy Program
Suzanne C. Madden, The LMC+ Consortium
With the goal of elucidating the effects of low metallicity on the star formation activity, feedback and interstellar medium of low metallicity environments, SOFIA has observed a 4…
Star Formation in the Extreme Galactic Center Environment
Mark R. Morris
Copious star formation occurs in the dense Central Molecular Zone (CMZ) of our Galaxy, but at a much smaller rate than occurs in a comparable mass of molecular gas in the Galactic…
Current and Future Space and Airborne Observatories for ISM Studies
Bernhard Schulz, Margaret Meixner
A tremendous amount of radiation is emitted by the Interstellar Medium in the mid- and far-infrared (3-500 μm) that represents the majority of the light emitted by a galaxy. In thi…