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 30 publications
The opaque heart of the galaxy IC 860: Analogous protostellar, kinematics, morphology, and chemistry
A technique to select the most obscured galaxy nuclei
APEX and NOEMA observations of H
CON-quest: Searching for the most obscured galaxy nuclei
ALCHEMI, an ALMA Comprehensive High-resolution Extragalactic Molecular Inventory: Survey presentation and first results from the ACA array
Discovery of methanimine (CH
Planck 's Dusty GEMS: VIII. Dense-gas reservoirs in the most active dusty starbursts at z ∼3
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
ALMA resolves the remarkable molecular jet and rotating wind in the extremely radio-quiet galaxy NGC 1377
A spectral stacking analysis to search for faint outflow signatures in z ∼6 quasars
Planck 's Dusty GEMS: VII. Atomic carbon and molecular gas in dusty starburst galaxies at z = 2 to 4
The hidden heart of the luminous infrared galaxy IC 860: I. A molecular inflow feeding opaque, extreme nuclear activity
Hidden or missing outflows in highly obscured galaxy nuclei?
Molecular gas in the northern nucleus of Mrk 273: Physical and chemical properties of the disc and its outflow
Major impact from a minor merger The extraordinary hot molecular gas flow in the Eye of the NGC 4194 Medusa galaxy
Planck's dusty GEMS V. Molecular wind and clump stability in a strongly lensed star-forming galaxy at z=2.2
Hidden molecular outflow in the LIRG Zw 049.057
Plancks dusty gems: VI. Multi-j co excitation and interstellar medium conditions in dusty starburst galaxies at z = 2 - 4*
Spatially Resolved CO SLED of the Luminous Merger Remnant NGC 1614 with ALMA
Planck's dusty GEMS: III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z = 1.5
Atomic hydrogen bridge fueling NGC 4418 with gas from VV 655
Luminous, pc-scale CO 6-5 emission in the obscured nucleus of NGC 1377
Planck's dusty GEMS IV. Star formation and feedback in a maximum starburst at z=3 seen at 60-pc resolution
Subarcsecond imaging of the water emission in Arp 220
Subarcsecond international LOFAR radio images of Arp 220 at 150 MHz: A kpc-scale star forming disk surrounding nuclei with shocked outflows
Deep ALMA imaging of the merger NGC 1614. Is CO tracing a massive inflow of non-starforming gas?
A low-luminosity type-1 QSO sample. IV. Molecular gas contents and conditions of star formation in three nearby Seyfert galaxies
Planck's Dusty GEMS. II. Extended [CII] emission and absorption in the Garnet at z=3.4 seen with ALMA
ACA CI observations of the starburst galaxy NGC 253
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