From the 5 of 91 papers with an AI index.
176 citations
- Centre National de la Recherche ScientifiqueFR24 papers
- Space Telescope Science InstituteUS20 papers
- Center for Astrophysics Harvard & SmithsonianUS18 papers
- University of ArizonaUS16 papers
- California Institute of TechnologyUS13 papers
- Goddard Space Flight CenterUS13 papers
- Instituto de Astrofísica de CanariasES13 papers
- Observatoire de la Côte d’AzurFR13 papers
- Jet Propulsion LaboratoryUS12 papers
- Massachusetts Institute of TechnologyUS12 papers
- Max Planck Institute for AstronomyDE12 papers
- National Astronomical Observatory of JapanJP12 papers
7 papers · 1 filter
Multiphase images of a powerful supernova-driven wind in the early Universe
Rebecca L. Davies, D. B. Fisher, R. Herrera-Camus +38
Galactic winds are considered a likely driver of rapid quenching in early massive galaxies, but until now there has been no direct evidence that such systems drive winds powerful e…
Clues to inside-out quenching in quiescent galaxies at : Age, Fe-, and Mg-abundance gradients from JWST-SUSPENSE
Chloe M. Cheng, Martje Slob, Mariska Kriek +16
[Abridged] Spatially resolved stellar populations of massive quiescent galaxies at cosmic noon provide powerful insights into quenching and assembly mechanisms. Previous photometri…
Surveying the Whirlpool at Arcseconds with NOEMA (SWAN). IV. Extent of active galactic nucleus feedback on the interstellar medium
Mallory D. Thorp, Antonio Usero, Frank Bigiel +19
Active Galactic Nuclei (AGN) are intertwined with galaxy evolution, injecting energy into the interstellar medium (ISM) that could regulate star formation as a galaxy evolves. Howe…
Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign
Ezequiel Albentosa-Ruiz, Jasmin E. Washington, Nicola Marchili +272
Sagittarius A* (Srg A*), the supermassive black hole at the center of the Milky Way, provides a unique laboratory to study accretion dynamics and plasma processes near the event ho…
An 18 - 25 GHz spectroscopic survey of southern hemisphere dense cores
Dariusz C. Lis, Karen Willacy, Liton Majumdar +3
We extended the radio K-band spectroscopic survey for organics in southern hemisphere dense cores by observing seven sources using NASA's Deep Space Network 70-m antenna in Canberr…
NE2025: An Updated Electron Density Model for the Galactic Interstellar Medium
S. K. Ocker, J. M. Cordes
Free electrons in the Galactic interstellar medium (ISM) disperse and scatter coherent radio waves, by amounts that depend on the distance to the radio source. Models of the Galact…