Author
Listed:
- M. Galeazzi
(University of Miami, Coral Gables, Florida 33124, USA)
- M. Chiao
(NASA Goddard Space Flight Center)
- M. R. Collier
(NASA Goddard Space Flight Center)
- T. Cravens
(University of Kansas)
- D. Koutroumpa
(Université Versailles St Quentin; CNRS/INSU, LATMOS-IPSL, Guyancourt 78280, France
Sorbonne Universités, UPMC Université Paris 06)
- K. D. Kuntz
(Johns Hopkins University)
- R. Lallement
(GEPI Observatoire de Paris, CNRS UMR 8111, Université Paris Diderot, 92190, Meudon, France)
- S. T. Lepri
(Oceanic and Space Sciences, University of Michigan)
- D. McCammon
(University of Wisconsin)
- K. Morgan
(University of Wisconsin)
- F. S. Porter
(NASA Goddard Space Flight Center)
- I. P. Robertson
(University of Kansas)
- S. L. Snowden
(NASA Goddard Space Flight Center)
- N. E. Thomas
(NASA Goddard Space Flight Center)
- Y. Uprety
(University of Miami, Coral Gables, Florida 33124, USA)
- E. Ursino
(University of Miami, Coral Gables, Florida 33124, USA)
- B. M. Walsh
(NASA Goddard Space Flight Center
Present address: Space Sciences Laboratory, University of California, Berkeley, California 94720, USA.)
Abstract
The contribution of solar-wind ions exchanging electrons with helium and hydrogen near the Sun is shown to be only about 40 per cent of the 1/4-keV X-ray flux observed in the Galactic plane; this supports the existence of a local ‘hot bubble’ filled with X-ray-emitting gas, accounting for the rest of the flux.
Suggested Citation
M. Galeazzi & M. Chiao & M. R. Collier & T. Cravens & D. Koutroumpa & K. D. Kuntz & R. Lallement & S. T. Lepri & D. McCammon & K. Morgan & F. S. Porter & I. P. Robertson & S. L. Snowden & N. E. Thomas, 2014.
"The origin of the local 1/4-keV X-ray flux in both charge exchange and a hot bubble,"
Nature, Nature, vol. 512(7513), pages 171-173, August.
Handle:
RePEc:nat:nature:v:512:y:2014:i:7513:d:10.1038_nature13525
DOI: 10.1038/nature13525
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