{"id":494748,"date":"2021-12-30T07:39:43","date_gmt":"2021-12-30T06:39:43","guid":{"rendered":"https:\/\/www.hashtag.al\/?p=494748"},"modified":"2021-12-30T07:41:50","modified_gmt":"2021-12-30T06:41:50","slug":"shperthimi-i-vrimes-se-zeze-sa-16-hena-kapet-ne-pamjet-me-gjitheperfshirese-ndonjehere-video","status":"publish","type":"post","link":"https:\/\/www.hashtag.al\/index.php\/2021\/12\/30\/shperthimi-i-vrimes-se-zeze-sa-16-hena-kapet-ne-pamjet-me-gjitheperfshirese-ndonjehere-video\/","title":{"rendered":"Shp\u00ebrthimi i vrim\u00ebs s\u00eb zez\u00eb sa 16 h\u00ebna kapet n\u00eb pamjet m\u00eb \u2018gjith\u00ebp\u00ebrfshir\u00ebse\u2019 ndonj\u00ebher\u00eb (Video)","gt_translate_keys":[{"key":"rendered","format":"text"}]},"content":{"rendered":"

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Nj\u00eb studim i ri i vrim\u00ebs s\u00eb zez\u00eb supermasive m\u00eb t\u00eb af\u00ebrt q\u00eb ushqehet n\u00eb m\u00ebnyr\u00eb aktive ka zbuluar se fenomeni hap\u00ebsinor l\u00ebshon flluska radioje t\u00eb cilat shtrihen n\u00eb hap\u00ebsira t\u00eb gjera kur ushqehet me gaz.<\/span><\/p>\n

N\u00eb nj\u00eb artikull t\u00eb botuar n\u00eb \u2018Nature Astronomy\u2019 m\u00eb 22 dhjetor, Dr. Benjamin McKinley nga Universiteti Curtin i Qendr\u00ebs Nd\u00ebrkomb\u00ebtare p\u00ebr K\u00ebrkimet e Radio-Astronomis\u00eb (ICRAR), i cili udh\u00ebhoqi studimin, tha se kjo pamje \u2018m\u00eb gjith\u00ebp\u00ebrfshir\u00ebse\u2019 deri m\u00eb sot tregon t\u00eb v\u00ebrtet\u00ebn e shkall\u00eb s\u00eb shqet\u00ebsimit n\u00eb hap\u00ebsir\u00eb \u200b\u200bt\u00eb shkaktuar kur vrimat e zeza supermasive ushqehen.<\/span><\/p>\n

Hulumtimi i McKinley ofron pamjet m\u00eb t\u00eb mira deri m\u00eb tani t\u00eb radiogalaktik\u00ebs fqinje m\u00eb t\u00eb af\u00ebrt t\u00eb Tok\u00ebs, Centaurus A, nj\u00eb sistem yjor i vendosur 12 milion\u00eb vite drit\u00eb larg me nj\u00eb vrim\u00eb t\u00eb zez\u00eb n\u00eb qend\u00ebr.<\/span><\/p>\n

Pamjet e kapura nga teleskopi Murchison Widefield Array (MWA) n\u00eb pjes\u00ebn e jashtme t\u00eb Australis\u00eb tregojn\u00eb flluska radioje t\u00eb cilat krijohen kur vrimat e zeza ushqehen me gaz q\u00eb bie dhe nxjerr materialin me shpejt\u00ebsi af\u00ebr drit\u00ebs.<\/span><\/p>\n

K\u00ebto flluska radio – ose ‘lobe’, si\u00e7 njihen nga astronom\u00ebt – duket se jan\u00eb 48 her\u00eb m\u00eb t\u00eb m\u00ebdha se sa vet\u00eb galaktika prit\u00ebse dhe aktualisht shtrihen tet\u00eb grad\u00eb n\u00eb t\u00eb gjith\u00eb qiellin, af\u00ebrsisht gjat\u00ebsia e 16 h\u00ebnave t\u00eb Tok\u00ebs t\u00eb vendosura krah p\u00ebr krah.<\/span><\/p>\n

Lobet formojn\u00eb \u2018nj\u00eb disk rreth vrim\u00ebs s\u00eb zez\u00eb, dhe nd\u00ebrsa l\u00ebnda shk\u00ebputet duke shkuar pran\u00eb vrim\u00ebs s\u00eb zez\u00eb, \u2018avion\u00eb\u2019 t\u00eb fuqish\u00ebm formohen n\u00eb t\u00eb dyja an\u00ebt e diskut, duke nxjerr\u00eb pjes\u00ebn m\u00eb t\u00eb madhe t\u00eb materialit p\u00ebrs\u00ebri n\u00eb hap\u00ebsir\u00eb, n\u00eb distanca ndoshta m\u00eb t\u00eb m\u00ebdha se nj\u00eb milion vite drit\u00eb\u2019, tha McKinley.<\/span><\/p>\n

Ai pretendoi se ky hulumtim kap\u00ebrcen kufizimet e studimeve ekzistuese.<\/span><\/p>\n

“V\u00ebzhgimet e m\u00ebparshme radio nuk mund t\u00eb p\u00ebrballonin shk\u00eblqimin e tejskajsh\u00ebm dhe holl\u00ebsit\u00eb e zon\u00ebs m\u00eb t\u00eb madhe q\u00eb rrethonte galaktik\u00ebn, por pamja jon\u00eb e re i kap\u00ebrcen k\u00ebto kufizime.”<\/em> – vuri n\u00eb dukje shkenc\u00ebtari.<\/span><\/p>\n