Pulsar Winds
Pulsar Winds is a high-energy astrophysical plasma outflow emanating from the magnetosphere of a rotating neutron star, distinguished by its relativistic particle content and strong electromagnetic fields driven by the star's rotational energy loss.
264
Publications
17.1K
Citations
916
Authors
344
Institutions
Publications per year
2017–2026
44
Variants
Pulsar Wind
Parents
264
The Evolution and Structure of Pulsar Wind Nebulae
Annual Review of Astronomy and Astrophysics · 2006 · 809 citations · Full text
Natural Sciences, Astronomy, Physics +13
A Periodically Active Pulsar Giving Insight into Magnetospheric Physics
M. Krämer, A. G. Lyne, J. T. O'Brien et al. · Science · 2006 · 516 citations · Full text
Reconnection in a Striped Pulsar Wind
The Astrophysical Journal · 2001 · 404 citations · Full text
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344
Max Planck Institute for Nuclear Physics
Heidelberg, Germany
23 h-index
140 publications
11.9K citations
Dublin Institute For Advanced Studies
Dublin, Ireland
22 h-index
26 publications
1.8K citations

Centre National de la Recherche Scientifique
Paris, France
19 h-index
202 publications
16.4K citations
Arcetri Astrophysical Observatory
Florence, Italy
17 h-index
35 publications
2.2K citations

Pennsylvania State University
State College, United States
14 h-index
29 publications
1.6K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
12 h-index
54 publications
2.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
12 h-index
18 publications
2.7K citations
Universitat de Barcelona
Barcelona, Spain
11 h-index
19 publications
515 citations
1–8 of 344
ApJ · 67 publications · 5.2K citations
39
h-index
44 publications · 2.9K citations
29
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41 publications · 2.6K citations
29
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Repository · 8 publications · 190 citations
8
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Repository · 8 publications · 566 citations
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