Showing 361–380 of 2,473 results
/ Date/ Name
Dec 19, 2024Supermassive black hole growth in hierarchically merging nuclear star clustersDec 18, 2024The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interactionDec 10, 2024Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic techniqueDec 6, 2024Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 MyrDec 5, 2024Overdensity of Lyman-Break Galaxy Candidates Around Hot Dust-Obscured GalaxiesDec 5, 2024The radio properties of the JWST-discovered AGNDec 5, 2024The cosmic globular cluster formation history in the E-MOSAICS simulationsDec 5, 2024Multi-wavelength picture of the misaligned BL Lac object 3C 371Dec 5, 2024Atmospheric molecular blobs shape up circumstellar envelopes of AGB starsDec 5, 2024CO-to-H$_2$ conversion factor and grain size distribution through the analysis of $α_\mathrm{CO}$-$q_\mathrm{PAH}$ relationDec 3, 2024The Multimodal Universe: Enabling Large-Scale Machine Learning with 100TB of Astronomical Scientific DataDec 3, 2024Wandering and escaping: recoiling massive black holes in cosmological simulationsDec 2, 2024The ionizing photon production efficiency of star-forming galaxies at $z\sim 4-10$Dec 1, 2024Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-Field ImagesNov 30, 2024An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclustersNov 29, 2024A New Look at Disk Winds and External Photoevaporation in the $σ$-Orionis ClusterNov 27, 2024SynthPop: A New Framework for Synthetic Milky Way Population GenerationNov 27, 2024Multiwavelength Properties of Infrared-Faint Radio Sources Based on Spectral Energy Distribution AnalysisNov 26, 2024New tools for studying planarity in galaxy satellite systems: Milky Way satellite planes are consistent with ΛCDMNov 26, 2024Dimming events of evolved stars due to clouds of molecular gas. Scenarios based on 3D radiation-hydrodynamics simulations with CO5BOLD