The quiescent X-ray emission of dwarf novae SSC_26
收藏ESA Earth Online2026-06-22 收录
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GTWe will make XMM observations of dwarf novae in their normalquiescent state. We select the brightest dwarf nova, SS Cyg, fora detailed spectral study with the RGS, and also the brightesteclipsing dwarf nova, HT Cas, allowing us to measure the locationof the Xray source.
