I-Space Research Institute ye-Russian Academy of Sciences (IKI RAS) yethule esinye sezithombe zokuqala ezidluliselwe eMhlabeni sisuka endaweni yokubuka i-Spektr-RG.
Iphrojekthi ye-Spektr-RG, siyakhumbula, ihloselwe ukufunda i-Universe ku-X-ray wavelength range. I-observatory ithwala izibonakude ezimbili ze-X-ray ezine-oblique incidence optics - ithuluzi laseRussia i-ART-XC kanye nensimbi ye-eRosita, eyakhiwe eJalimane.
Ukwethulwa ngempumelelo kwendawo yokubuka izinto kwenzeke ngoJulayi 13 nonyaka. Manje idivayisi itholakala endaweni ye-Lagrange L2, lapho ihlola isibhakabhaka sonke ngemodi yokuskena.
Isithombe sokuqala sibonisa inhlolovo yesifunda esimaphakathi somthala wethu ngesibonakude se-ART-XC ebangeni lamandla aqinile. Indawo yesithombe ingama-degrees square angu-40. Imibuthano ikhombisa imithombo yemisebe ye-X-ray. Phakathi kwabo kukhona ishumi nambili elalingaziwa ngaphambilini; mhlawumbe lezi amasistimu kanambambili accreting anenkanyezi ye-neutron noma imbobo emnyama.
Isithombe sesibili sibonisa iqoqo lomthala we-Coma kumlaza i-Coma Berenices. Isithombe sitholwe yisibonakude se-ART-XC ebangeni eliqinile le-X-ray 4–12 keV. Imibuthano egxilile ikhombisa izindawo zokukhanya okuphansi kakhulu. Isithombe sesithathu siyiqoqo elifanayo lemithala, kodwa ngeso le-eRosita.
Isithombe sesine imephu ye-X-ray yengxenye ye-galactic disk ("i-Galactic Ridge") etholwe yisibonakude se-eRosita. Imithombo eminingi ye-X-ray etholakala emthaleni wethu, kanye naleyo eqhelelene nathi futhi ebonwa “ngokudluliselana”, iye yaqoshwa lapha.
Ekugcineni, isithombe sokugcina sibonisa “imbobo ye-Lokman” - indawo eyingqayizivele esibhakabhakeni lapho ukumuncwa kwemisebe ye-X ray yi-interstellar medium yomthala wethu kufinyelela inani elincane. Lokhu kwenza kube nokwenzeka ukutadisha ama-quasars akude namaqoqo omthala anokuzwela kwamarekhodi.
Source: 3dnews.ru