Isibonakude saseRussia i-ART-XC esiku-Spektr-RG space observatory sesiqale uhlelo lwaso lokuqala lwesayensi. Ngesikhathi sokuskena kokuqala “kweqhubu” elimaphakathi lomthala i-Milky Way, kutholwe umthombo omusha we-X-ray, obizwa nge-SRGA J174956-34086.
Phakathi naso sonke isikhathi sokubhekwa, isintu siye sathola imithombo engaba yisigidi yemisebe ye-X ray, futhi inqwaba kuphela yayo enamagama awo. Ezimweni eziningi, ziqanjwa ngendlela efanayo, futhi isisekelo segama yigama le-observatory eyathola umthombo. Ngemuva kokutholakala komthombo omusha, ososayensi kuzofanele baqhubeke nocwaningo oluzosiza ekutholeni uhlobo lwawo. Umthombo ungaba i-quasar ekude noma isistimu yezinkanyezi eseduze enenkanyezi ye-neutron noma imbobo emnyama.
Ukuze bathole indawo ngokunembile le nto, ososayensi babona umthombo wemisebe evela kwesinye isibonakude. I-Neil Gehrels Swift X-ray telescope, i-XRT, enokulungiswa okungcono kwe-angular, yasetshenziswa. Umthombo wemisebe kuma-X ray athambile wabonakala ufiphele kunakuma-X ray aqinile. Lokhu kwenzeka uma umthombo wemisebe utholakala ngemuva kwamafu egesi ephakathi kwezinkanyezi nothuli.
Ngokuzayo, ososayensi bazozama ukuthola i-optical spectra ezokwenza kube nokwenzeka ukunquma uhlobo lomthombo we-X-ray otholiwe. Uma lokhu kwehluleka, i-ART-XC izoqhubeka nokuhlola izindawo ukuze ithole izinto ezibuthakathaka. Naphezu kwenani elizayo lomsebenzi, kuyaphawulwa ukuthi isibonakude saseRussia i-ART-XC sesivele sishiye uphawu lwaso kumakhathalogi emithombo ye-X-ray.
Source: 3dnews.ru