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

PhD

Giovanni Stel
PhD @ INAF-Osservatorio astronomico di Brera
E-mail: giovanni.stel_AT_inaf.it - giovanni.stel_AT_gmail.com



PhD

Yi Zhang
PhD @ MPE
E-mail: yi_zhang_AT_smail.nju.edu.cn



PhD

Xueying Zheng
PhD @ MPE
E-mail: zhengxy_AT_bao.ac.cn



Post Doc

Heshou Zhang
Post Doc @ INAF-Osservatorio astronomico di Brera
E-mails: heshou.zhang_AT_inaf.it - heshouzhang.astrophy_AT_gmail.com



Post Doc

Nicola Locatelli
Post Doc @ OAB
E-mail: nicola.locatelli_AT_inaf.it



Post Doc

Samaresh Mondal
Post Doc @ INAF-Osservatorio astronomico di Brera
E-mail: samaresh.mondal_AT_inaf.it



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



Secretaries

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



Petra Dell’Arme
Secretary @ INAF-Osservatorio astronomico di Brera
E-mail: petra.dellarme_AT_inaf.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