Duba wurin da ke ƙasa sannan ka amsa tambayar daga baya a cikin harshe ɗaya kamar yadda wurin yake:  Passage: A shekara ta 2001, lura a X-ray wavelengths ta Chandra X-ray Observatory ya bayyana kasancewar gas mai zafi sosai a cikin NGC 6543 tare da zafin jiki na 1.7 × 106 K. Ana tunanin cewa gas mai zafi yana haifar da mu'amala mai ƙarfi na iska mai sauri tare da kayan da aka fitar a baya. Wannan hulɗar ta ɓoye kumfa na ciki na nebula. Binciken Chandra ya kuma bayyana tushen ma'ana a matsayin tauraron tsakiya. Hasken wannan tushen ya faɗaɗa zuwa ɓangaren ɓangaren X-ray, zuwa 0.5<unk>1.0 keV. Tauraruwa tare da zafin jiki na photospheric na kimanin 100000 K ba za a sa ran ya fitar da karfi a cikin rayukan X-ray mai wuya ba, don haka kasancewarsu wani abu ne mai ban mamaki. Zai iya nuna kasancewar babban diski mai yawan zafin jiki a cikin tsarin tauraron binary. Bayanin X-ray mai wuya ya kasance mai ban sha'awa fiye da shekaru goma bayan haka: An haɗa ido na Cat a cikin binciken Chandra na 2012 na taurari 21 na taurari na tauraron dan adam (CSPNe) a cikin unguwar hasken rana, wanda ya gano: "Duk amma daya daga cikin X-ray point sources da aka gano a CSPNe suna nuna hotunan X-ray waɗanda suka fi wuya fiye da yadda ake tsammani daga hot (~100000 K) tauraron tauraron dan adam, mai yiwuwa yana nuna babban mita na abokan binary zuwa CSPNe. Sauran bayani mai yiwuwa sun hada da iska mai cin gashin kanta ko PN mai yawa".  Tambaya: Menene Chandra X Ray Observatory ya bayyana?
tashin hankali na iska mai sauri tare da kayan da aka fitar da shi a baya