Showing 1–20 of 37 results
/ Date/ Name
Jul 24, 2024Chemical tracers of a highly eccentric AGB-main sequence star binaryJul 19, 2024Star Formation in Extreme Environments: A 200 pc High Velocity Gas Stream in the Galactic CentreFeb 1, 2024Ordered magnetic fields around the 3C 84 central black holeSep 19, 2022Ammonia in the interstellar medium of a starbursting disc at z=2.6Dec 15, 2021ALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first resultsFeb 23, 2021The physical and chemical structure of high-mass star-forming regions. Unraveling chemical complexity with the NOEMA large program "CORE"Oct 11, 2019Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot coreOct 29, 2018ALMA reveals potential evidence for spiral arms, bars, and rings in high-redshift submillimeter galaxiesApr 17, 2018The search for high-mass protostars with ALMA revealed up to kilo-parsec scales (SPARKS): I. Indication for a centrifugal barrier in the environment of a single high-mass envelopeMar 9, 2017ALMA survey of massive cluster progenitors from ATLASGAL. Limited fragmentation at the early evolutionary stage of massive clumpsMar 16, 2016The redshift distribution of dusty star forming galaxies from the SPT surveyDec 13, 2015The first Galaxy scale hunt for the youngest high-mass protostarsNov 16, 2015A study of the C$_3$H$_2$ isomers and isotopologues: first interstellar detection of HDCCCFeb 14, 2014A sub-arcsecond study of the hot molecular core in G023.01-00.41Oct 3, 2013MALT90: The Millimetre Astronomy Legacy Team 90 GHz SurveySep 20, 2013PO and PN in the wind of the oxygen-rich AGB star IK TauMay 8, 2013Interstellar detection of c-C3D2Mar 11, 2013ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxiesMar 11, 2013Dusty starburst galaxies in the early Universe as revealed by gravitational lensingFeb 27, 2013Dust-forming molecules in VY Canis Majoris (and Betelgeuse)