9 citations · 28 across the 5 of their papers we have counts for
7 papers
A multi-scale view of molecular gas and magnetic fields in the Antennae galaxies
Akhil Lasrado, Enrique Lopez-Rodriguez, Claudia Cicone +5
Major mergers are transformative events in galaxy evolution, dynamically reshaping the stellar and gas makeup of the hosts, as well as the galaxy-scale magnetic fields (B-fields) t…
The extended molecular gas of the Circinus galaxy and NGC 1097 as seen by APEX
Akhil Lasrado, Claudia Cicone, Axel Weiss
The outer region of the interstellar medium (ISM) is witness to dynamically important events in a galaxy's evolutionary history such as outflows, inflows, tidal interactions, and m…
Outflowing shocked gas dominates the NIR H emission from the dual AGN NGC6240
J. Carlsen, C. Cicone, B. Hagedorn +10
[Abridged] We present a multi-line study of the kinematics of the molecular and ionised gas phases in the central 2 kpc of NGC6240, based on JWST/NIRSpec and ALMA observations. We…
investigation of cores and filamentary structures in L1251 located in the Cepheus flare
Divyansh Dewan, Archana Soam, Guo-Yin Zhang +3
Context: Molecular clouds are the prime locations of star formation. These clouds contain filamentary structures and cores which are crucial in the formation of young stars. Aims:…
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies
Daizhong Liu, Amelie Saintonge, Caroline Bot +25
Understanding the physical processes that regulate star formation and galaxy evolution are major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunitie…
Molecular gas scaling relations for local star-forming galaxies in the low- regime
B. Hagedorn, C. Cicone, M. Sarzi +7
We derived molecular gas fractions () and depletion times () for 353 galaxies representative of the…
Spiral Structure and Massive Star formation in the Hub-Filament-System G326.27-0.49
Bhaswati Mookerjea, V. S. Veena, Rolf Guesten +2
Hub-filament systems (HFSs) are potential sites of formation of star clusters and high mass stars. To understand the HFSs and to provide observational constraints on current theori…