English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Recently, the magnetar Swift J1834.9$-$0846 is reported to have a possiblewind nebula. It is shown that both the magnetar and its wind nebula areunderstandable in the wind braking scenario. The magnetar's rotational energyloss rate is not enough to power the particle luminosity. The required particleluminosity should be about $10^{36} \,\rm erg \,s^{-1}$ to $10^{38} \,\rm erg\,s^{-1}$. It is obtained in three different approaches: considering windbraking of Swift J1834.9$-$0846; the spectral and spatial observations of thewind nebula; and an empirical upper bound on wind nebula X-ray luminosity. Thenebula magnetic field is about $10^{-4} \,\rm G$. The possible wind nebula ofSwift J1834.9$-$0846 should be a magnetar wind nebula. It is powered by themagnetic energy release of the magnetar.

On the possible wind nebula of magnetar Swift J1834.9-0846: a magnetism-powered synchrotron nebula