Detection of large-scale X-ray bubbles in the Milky Way halo
Detection of large-scale X-ray bubbles in the Milky Way halo
About this item
Full title
Author / Creator
Predehl, P. , Sunyaev, R. A. , Becker, W. , Brunner, H. , Burenin, R. , Bykov, A. , Cherepashchuk, A. , Chugai, N. , Churazov, E. , Doroshenko, V. , Eismont, N. , Freyberg, M. , Gilfanov, M. , Haberl, F. , Khabibullin, I. , Krivonos, R. , Maitra, C. , Medvedev, P. , Merloni, A. , Nandra, K. , Nazarov, V. , Pavlinsky, M. , Ponti, G. , Sanders, J. S. , Sasaki, M. , Sazonov, S. , Strong, A. W. and Wilms, J.
Publisher
London: Nature Publishing Group UK
Journal title
Language
English
Formats
Publication information
Publisher
London: Nature Publishing Group UK
Subjects
More information
Scope and Contents
Contents
The halo of the Milky Way provides a laboratory to study the properties of the shocked hot gas that is predicted by models of galaxy formation. There is observational evidence of energy injection into the halo from past activity in the nucleus of the Milky Way
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–
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; however, the origin of this energy (star formation or supermassive-bl...
Alternative Titles
Full title
Detection of large-scale X-ray bubbles in the Milky Way halo
Authors, Artists and Contributors
Author / Creator
Sunyaev, R. A.
Becker, W.
Brunner, H.
Burenin, R.
Bykov, A.
Cherepashchuk, A.
Chugai, N.
Churazov, E.
Doroshenko, V.
Eismont, N.
Freyberg, M.
Gilfanov, M.
Haberl, F.
Khabibullin, I.
Krivonos, R.
Maitra, C.
Medvedev, P.
Merloni, A.
Nandra, K.
Nazarov, V.
Pavlinsky, M.
Ponti, G.
Sanders, J. S.
Sasaki, M.
Sazonov, S.
Strong, A. W.
Wilms, J.
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_miscellaneous_2469090730
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_2469090730
Other Identifiers
ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/s41586-020-2979-0
