Avtory i prava: Hillary Mathis i N.A.Sharp
(Nacional'naya Opticheskaya Astronomicheskaya Observatoriya
(NOAO)),
Associaciya universitetov po issledovaniyam
v oblasti astronomii (AURA),
Nacional'nyi nauchnyi fond (NSF)
Poyasnenie:
Pochemu central'naya chast' galaktiki
M94 takaya yarkaya?
Vokrug yadra spiral'noi galaktiki
M94 imeetsya kol'cevaya oblast', soderzhashaya nedavno sformirovannye zvezdy,
kotoraya blagodarya svoemu intensivnomu svecheniyu pridaet galaktike takoi
neobychnyi vid.
Osnovnoi
gipotezoi dlya ob'yasneniya
vspyshki zvezdoobrazovaniya, rasprostranyayusheisya naruzhu v vide kol'ca,
yavlyaetsya vrashenie peremychki galaktiki
(vytyanutoi i zaputannoi struktury zvezd).
Galaktika M94, izobrazhennaya na
risunke, obrabotannom cifrovym metodom, imeet protyazhennost'
primerno 30 000 svetovyh let i nahoditsya ot nas na rasstoyanii 15 millionov
svetovyh let.
Ee mozhno uvidet' v
nebol'shoi teleskop v sozvezdii
Gonchih Psov.
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Publikacii s klyuchevymi slovami:
spiral galaxy - starburst - M 94 - spiral'naya galaktika - vspyshka zvezdoobrazovaniya
Publikacii so slovami: spiral galaxy - starburst - M 94 - spiral'naya galaktika - vspyshka zvezdoobrazovaniya | |
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