Sabine König
Sabine's research is focused on the physical properties in the interstellar medium in nearby galaxies. For her work she uses ground-based telescopes all over the world like ALMA, NOEMA and the SMA to study the connection between molecular gas, star formation and AGN activity in close-by minor mergers.
Showing 39 publications
An Imaging and Spectroscopic Exploration of the Dusty Compact Obscured Nucleus Galaxy Zw 049.057
The ALCHEMI Atlas: Principal Component Analysis Reveals Starburst Evolution in NGC 253
The fountain of the luminous infrared galaxy Zw049.057 as traced by its OH megamaser
A multi-wavelength overview of the giant spiral UGC 2885
A spectacular galactic scale magnetohydrodynamic powered wind in ESO 320-G030
The opaque heart of the galaxy IC 860: Analogous protostellar, kinematics, morphology, and chemistry
A technique to select the most obscured galaxy nuclei
Discovery of methanimine (CH<inf>2</inf>NH) megamasers toward compact obscured galaxy nuclei
Planck 's Dusty GEMS: VIII. Dense-gas reservoirs in the most active dusty starbursts at z ∼3
CON-quest: Searching for the most obscured galaxy nuclei
VV 655 and NGC 4418: Implications of an interaction for the evolution of a LIRG
Star cluster formation in the most extreme environments: Insights from the HiPEEC survey
Hidden or missing outflows in highly obscured galaxy nuclei?
Planck 's Dusty GEMS: VII. Atomic carbon and molecular gas in dusty starburst galaxies at z = 2 to 4
A spectral stacking analysis to search for faint outflow signatures in z ∼6 quasars
Hidden molecular outflow in the LIRG Zw 049.057
Luminous, pc-scale CO 6-5 emission in the obscured nucleus of NGC 1377
Atomic hydrogen bridge fueling NGC 4418 with gas from VV 655
Spatially Resolved CO SLED of the Luminous Merger Remnant NGC 1614 with ALMA
Subarcsecond imaging of the water emission in Arp 220
Deep ALMA imaging of the merger NGC 1614. Is CO tracing a massive inflow of non-starforming gas?
ACA CI observations of the starburst galaxy NGC 253
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