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Flows of hot plasma connecting the Milky Way center to the corona, halo and beyond
People - Contact us

Principal Investigator

Gabriele Ponti
First researcher @ INAF-Osservatorio astronomico di Brera
Visiting scientist @ Max Planck for Extraterrestrial Physics
E-mails: gabriele.ponti_AT_inaf.it - ponti_AT_mpe.mpg.de


Lorella Galliani
Secretary @ INAF-Osservatorio astronomico di Brera
E-mails: lorella.galliani_AT_inaf.it


Xueying Zheng
E-mails: zhengxy_AT_bao.ac.cn

Post Doc

Konstantina Anastasopoulou
PhD @ INAF-Osservatorio astronomico di Brera
E-mails: kanast_ARphysics.uoc.gr

Post Doc

Nicola Locatelli
E-mails: nicola.locatelli2_AT_unibo.it


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