An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre.


Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
03 2019
Historique:
received: 06 11 2018
accepted: 30 01 2019
entrez: 22 3 2019
pubmed: 22 3 2019
medline: 22 3 2019
Statut: ppublish

Résumé

Evidence has mounted in recent decades that outflows of matter and energy from the central few parsecs of our Galaxy have shaped the observed structure of the Milky Way on a variety of larger scales

Identifiants

pubmed: 30894726
doi: 10.1038/s41586-019-1009-6
pii: 10.1038/s41586-019-1009-6
doi:

Types de publication

Journal Article Research Support, U.S. Gov't, Non-P.H.S. Research Support, Non-U.S. Gov't

Langues

eng

Sous-ensembles de citation

IM

Pagination

347-350

Commentaires et corrections

Type : CommentIn

Auteurs

G Ponti (G)

Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany. gabriele.ponti@inaf.it.
INAF-Osservatorio Astronomico di Brera, Merate, Italy. gabriele.ponti@inaf.it.

F Hofmann (F)

Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany.

E Churazov (E)

Max-Planck-Institut für Astrophysik, Garching, Germany.
Space Research Institute (IKI), Moscow, Russia.

M R Morris (MR)

Department of Physics and Astronomy, University of California, Los Angeles, CA, USA.

F Haberl (F)

Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany.

K Nandra (K)

Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany.

R Terrier (R)

Unité mixte de recherche Astroparticule et Cosmologie, Paris, France.

M Clavel (M)

Université Grenoble Alpes, CNRS, IPAG, Grenoble, France.

A Goldwurm (A)

Unité mixte de recherche Astroparticule et Cosmologie, Paris, France.
Département d'Astrophysique (DAp), IRFU/DRF/CEA-Saclay, Gif-sur-Yvette, France.

Classifications MeSH