What’s the storyline?: may 05, 2022 cosmicnoon_r6mdvbMay 9, 2022 Study of the hot intracluster medium Plasma physics of the intracluster medium The morphology of the cold molecular clouds and The SEDIGISM survey: Molecular cloud morphology. II. Integrated source properties The deep gravitational potential that holds them all together Deep Potential: Recovering the gravitational potential from a snapshot of phase space
What’s the storyline? :april20,2022 cosmicnoon_r6mdvbApril 26, 2022 Relationship between the information content in life and the information content in the Universe: Biocosmology: Towards the birth of a new science Finding civilizations with Dyson spheres: Infrared and Optical Detectability of Dyson Spheres at White Dwarf Stars Local habitable environments (our sun and Proxima Centauri) : Detection of stellar-like abundance anomalies in the slow solar wind The high energy spectrum of Proxima Centauri simultaneously observed at X-ray and FUV wavelengths Exploring the Milky Way’s family tree: A new member of the Milky Way’s family tree: Characterizing the Pontus merger of our Galaxy A photon from the FUV background knocks you out. Uh oh! The Far Ultraviolet Background
astro-ph astronomy astroph What’s the storyline? :april21,2022 cosmicnoon_r6mdvbApril 24, 2022 James webb and blackholes: The Age of Discovery with the James Webb: Excavating the Spectral Signatures of the First Massive Black Holes Blackholes and supersonic turbulence : Signature of Supersonic Turbulence in Galaxy Clusters Revealed by AGN-driven Hα Filaments Feedback and Massive stars: A Massive Star is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars Most massive stars are in binaries, but where do they go after becoming magnetars? : Where are the magnetar binary companions? Candidates from a comparison with binary population synthesis predictions Young stars and leaking Lyman photons: The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5