. . . . . "1116563623"^^ . . . . . "\uCD08\uC810\uADFC\uAC70\uC131"@ko . . . . . . . . . . . "\uCD08\uC810\uADFC\uAC70\uC131(\uC601\uC5B4: Super-AGB star)\uC774\uB780 \uC810\uADFC\uAC70\uC131\uAC00\uC9C0\uC640 \uC801\uC0C9 \uCD08\uAC70\uC131\uC758 \uC911\uAC04 \uC131\uC9C8\uC774 \uB098\uD0C0\uB098\uB294 \uD56D\uC131\uC774\uB2E4. \uBC31\uC0C9\uC65C\uC131\uC73C\uB85C \uC77C\uC0DD\uC758 \uB05D\uC744 \uB9FA\uB294 \uD56D\uC131\uACFC \uC911\uC2EC\uD575 \uBD95\uAD34 \uCD08\uC2E0\uC131\uC73C\uB85C \uB05D\uC744 \uB9DE\uC774\uD558\uB294 \uD56D\uC131 \uC911\uAC04\uD615\uC758 \uC9C4\uD654 \uACFC\uC815\uC5D0\uC11C \uB098\uD0C0\uB09C\uB2E4. \uD56D\uC131 \uC9C4\uD654 \uBAA8\uD615\uC5D0 \uB530\uB974\uBA74 \uC774\uB4E4\uC740 \uCC98\uC74C\uC5D0 \uC9C8\uB7C9\uC774 7.5~9.25M\u2609\uC774\uC5C8\uC9C0\uB9CC, \uC8FC\uACC4\uC5F4\uC744 \uB5A0\uB09C \uD6C4 \uD575\uC758 \uC218\uC18C\uC640 \uD5EC\uB968\uC774 \uACE0\uAC08\uB418\uC5B4 \uD06C\uAC8C \uBD80\uD480\uC5B4\uC624\uB974\uBA70 \uD45C\uBA74\uC774 \uCC28\uAC00\uC6CC\uC9C0\uACE0 \uBC1D\uC544\uC9C4 \uC0C1\uD0DC\uB2E4."@ko . . . . . . . . . "A super-AGB star is a star with a mass intermediate between those that end their lives as a white dwarf and those that end with a core collapse supernova, and properties intermediate between asymptotic giant branch (AGB) stars and red supergiants. They have initial masses of 7.5\u20139.25 M\u2609 in stellar-evolutionary models, but have exhausted their core hydrogen and helium, left the main sequence, and expanded to become large, cool, and luminous."@en . . . "\uCD08\uC810\uADFC\uAC70\uC131(\uC601\uC5B4: Super-AGB star)\uC774\uB780 \uC810\uADFC\uAC70\uC131\uAC00\uC9C0\uC640 \uC801\uC0C9 \uCD08\uAC70\uC131\uC758 \uC911\uAC04 \uC131\uC9C8\uC774 \uB098\uD0C0\uB098\uB294 \uD56D\uC131\uC774\uB2E4. \uBC31\uC0C9\uC65C\uC131\uC73C\uB85C \uC77C\uC0DD\uC758 \uB05D\uC744 \uB9FA\uB294 \uD56D\uC131\uACFC \uC911\uC2EC\uD575 \uBD95\uAD34 \uCD08\uC2E0\uC131\uC73C\uB85C \uB05D\uC744 \uB9DE\uC774\uD558\uB294 \uD56D\uC131 \uC911\uAC04\uD615\uC758 \uC9C4\uD654 \uACFC\uC815\uC5D0\uC11C \uB098\uD0C0\uB09C\uB2E4. \uD56D\uC131 \uC9C4\uD654 \uBAA8\uD615\uC5D0 \uB530\uB974\uBA74 \uC774\uB4E4\uC740 \uCC98\uC74C\uC5D0 \uC9C8\uB7C9\uC774 7.5~9.25M\u2609\uC774\uC5C8\uC9C0\uB9CC, \uC8FC\uACC4\uC5F4\uC744 \uB5A0\uB09C \uD6C4 \uD575\uC758 \uC218\uC18C\uC640 \uD5EC\uB968\uC774 \uACE0\uAC08\uB418\uC5B4 \uD06C\uAC8C \uBD80\uD480\uC5B4\uC624\uB974\uBA70 \uD45C\uBA74\uC774 \uCC28\uAC00\uC6CC\uC9C0\uACE0 \uBC1D\uC544\uC9C4 \uC0C1\uD0DC\uB2E4."@ko . . "A super-AGB star is a star with a mass intermediate between those that end their lives as a white dwarf and those that end with a core collapse supernova, and properties intermediate between asymptotic giant branch (AGB) stars and red supergiants. They have initial masses of 7.5\u20139.25 M\u2609 in stellar-evolutionary models, but have exhausted their core hydrogen and helium, left the main sequence, and expanded to become large, cool, and luminous."@en . . . "4300"^^ . . . "Super-AGB star"@en . . . . . . . "64411788"^^ .