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Flows of hot plasma connecting the Milky Way center to the corona, halo and beyond
 
 

News
11/11/2021 - ISM absorption
In MODELS section (link: models) you can find data from the article: "disnht: absorption from a distribution of column density" (Locatelli, Ponti and Bianchi, A&A, submitted 2021).

05/07/2021 - Marcel Grossmann Award
MPE shares institutional Marcel Grossmann Award for development of eROSITA aboard SRG - on MPE web site

09/12/2020 - Heritage program with XMM
Xmm-Newton, due italiani al comando - on Media Inaf

09/12/2020 - eROSITA bubbles
Sterminata clessidra di gas caldo nella Via Lattea - on Media Inaf
eROSITA finds large-scale bubbles in the halo of the Milky Way - on MPE web site
Detection of large-scale X-ray bubbles in the Milky Way halo - on Nature web site

10/09/2020 - New people in our team: Xueying Zheng will start in a week her PhD at Max Planck Institute for Extraterrestrial Physics (MPE) in Garching, Konstantina Anastasopoulou will start her post doc at the end of the month in Merate - INAF-Osservatorio Astronomico di Brera and Nicola Locatelli will start his post doc at MPE at the end of the year. Click here to read more ...

19/06/2020 - eROSITA press release
Il cielo X come non l’avete mai visto - on Media Inaf
Our deepest view of the X-ray sky - on MPE web site

 
 
 

This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation
programme (grant agreement No. [865637])

  
  
Banner image: The central regions of our galaxy, the Milky Way, seen in X-rays by ESA’s XMM-Newton X-ray observatory - Date: 20 August 2015 - XMM-Newton Satellite - Copyright: ESA/XMM-Newton/G. Ponti et al. 2015 - Web site credit: G. Ponti - M.R. Panzera