Showing 1–20 of 130 results
/ Date/ Name
Oct 7, 2024The Green Monster hiding in front of Cas A: JWST reveals a dense and dusty circumstellar structure pockmarked by ejecta interactionsSep 12, 2012The dust energy balance in the edge-on spiral galaxy NGC 4565Nov 17, 2016The interstellar medium in Andromeda's dwarf spheroidal galaxies: II. Multi-phase gas content and ISM conditionsSep 12, 2014High-resolution, 3D radiative transfer modeling : I. The grand-design spiral galaxy M51Feb 17, 2014The applicability of FIR fine-structure lines as Star Formation Rate tracers over wide ranges of metallicities and galaxy typesApr 22, 2016The interstellar medium in Andromeda's dwarf spheroidal galaxies: I. Content and origin of the interstellar dustJun 5, 2019The dust content of the Crab NebulaNov 2, 2016The dust mass in Cassiopeia A from a spatially resolved Herschel analysisJun 2, 2020JINGLE -- IV. Dust, HI gas and metal scaling laws in the local UniverseApr 5, 2012Herschel and JCMT observations of the early-type dwarf galaxy NGC 205May 18, 2010The complex interplay of dust and star light in spiral galaxy discsJun 3, 2011The Herschel Virgo Cluster Survey. IX. Dust-to-gas mass ratio and metallicity gradients in four Virgo spiral galaxiesFeb 1, 2024From total destruction to complete survival: Dust processing at different evolutionary stages in the supernova remnant Cassiopeia AApr 13, 2023Far-infrared Polarization of the Supernova Remnant Cassiopeia A with SOFIA HAWC+Oct 31, 2018A Catalogue of Galactic Supernova Remnants in the far-infrared: revealing ejecta dust in pulsar wind nebulaeJan 13, 2022B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens MainAug 28, 2013The Herschel Virgo Cluster Survey XIV: transition-type dwarf galaxies in the Virgo clusterMar 25, 2013Herschel Exploitation of Local Galaxy Andromeda (HELGA) III: The Star Formation Law in M31Apr 24, 2025The ALMA-CRISTAL survey: weak evidence for star-formation driven outflows in $z\sim5$ main-sequence galaxiesMar 17, 2025JWST/MIRI detects the dusty SN1993J about 30 years after explosion