094013
收藏DataCite Commons2026-03-09 更新2026-05-03 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/094013.html
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资源简介：
The presence of magnetically confined winds has been detected in many massivestars. The predictions for their X-ray emission generally fits the observationsbut there is a set of outliers. Auroral phenomena could be responsible for thisoverluminosity. However to ascertain this scenario and constrain this newprocess stars with known auroral radio emission should be observed in X-rays. [truncated! Please see actual data for full text]
提供机构：
European Space Agency
创建时间：
2026-03-09
