088284
收藏Mendeley Data2024-05-23 更新2024-06-27 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/xmm-newton/088284.html
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We aim to determine the frequency and characteristics of X-ray emission from RV Tau variables stars. Only one RV Tau variable star has been targeted by modern X- ray observatories and its detected X-ray emission is surprising and difficult to understand. We request 140 ks to study a pilot sample of four RV Tau variable stars in order to establish if X-ray emission is ubiquitous amongst these luminous and pulsating stars. The requested observations would determine the characteristics of any X-ray emission and help identify the origin of the X-ray emission. As known and suspected binary systems discovering X-ray emission from these stars can open new windows into binary evolution at their intermediate stages. [truncated! Please see actual data for full text]
创建时间:
2024-05-18



