Paul P. Plucinsky

3 ta ish

Center for Astrophysics Harvard & Smithsonian

1. XRISM Reveals Low Nonthermal Pressure in the Core of the Hot, Relaxed Galaxy Cluster A2029

   M. Audard, Hisamitsu Awaki, Ralf Ballhausen +97

   Maqola20254 iqtibos

   ABIABI:AkademIndex/2026.other.470740

2. XRISM Forecast for the Coma Cluster: Stormy, with a Steep Power Spectrum

   M. Audard, Hisamitsu Awaki, Ralf Ballhausen +97

   Maqola20254 iqtibos

   ABIABI:AkademIndex/2026.other.470741

3. XRISM Constraints on Unidentified X-Ray Emission Lines, Including the 3.5 keV Line, in the Stacked Spectrum of 10 Galaxy Clusters

   M. Audard, Hisamitsu Awaki, Ralf Ballhausen +97

   MaqolaOAOchiq kirishGalaxies: Formation, Evolution, PhenomenaThe Astrophysical Journal Letters20250 iqtibos

   ABIABI:AkademIndex/2025.article.002537