Iteleskopu ye-ART-XC yaseRashiya ekhwele kwindawo yokujonga indawo ye-Spektr-RG sele iqalisile inkqubo yayo yokuqala yesayensi. Ngethuba lokuskena kokuqala "kwe-bulge" ephakathi kwe-Milky Way galaxy, umthombo omtsha we-X-ray wafunyanwa, obizwa ngokuba yi-SRGA J174956-34086.
Ngalo lonke ixesha lokuphononongwa, uluntu luye lwafumanisa malunga nesigidi semithombo ye-X-reyi, kwaye liqela kuphela elinamagama awo. Kwiimeko ezininzi, zibizwa ngokufanayo, kwaye isiseko segama ligama le-observatory eyafumanisa umthombo. Emva kokufunyanwa komthombo omtsha, izazinzulu kuya kufuneka ziqhubeke nophando oluya kunceda ukufumanisa ubunjani bayo. Umthombo unokuba yi-quasar ekude okanye inkqubo yeenkwenkwezi ekufutshane eneenkwenkwezi ze-neutron okanye umngxuma omnyama.
Ukufumana indawo echanekileyo, izazinzulu zabona umthombo wemitha yemitha kwenye iteleskopu. Iteleskopu ye-X-ray ye-Neil Gehrels Swift, i-XRT, enesisombululo esingcono se-angular, yasetyenziswa. Umthombo wemitha okwiiX-reyi ezithambileyo wabonakala umnyama kuneeX-reyi ezinzima. Oku kwenzeka ukuba umthombo wemitha ubekwe emva kwamafu egesi ye-interstellar kunye nothuli.
Kwixesha elizayo, izazinzulu ziya kuzama ukufumana i-optical spectra eya kwenza kube lula ukumisela uhlobo lomthombo we-X-ray ofunyenweyo. Ukuba oku akuphumeleli, i-ART-XC iya kuqhubeka ukuhlola iindawo ukufumana izinto ezibuthathaka. Nangona inani elizayo lomsebenzi, kuyaphawulwa ukuba i-telescope yaseRashiya ye-ART-XC sele ishiye uphawu lwayo kwiikhathalogu zemithombo ye-X-ray.
umthombo: 3dnews.ru