KimAnt ๐Ÿฅฆ

KimAnt ๐Ÿฅฆ

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KimAnt ๐Ÿฅฆ

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  • 2022 ์ค‘๋ ฅํŒŒ, ์ˆ˜์น˜์ƒ๋Œ€๋ก  ์—ฌ๋ฆ„ํ•™๊ต - 4. ๋ณ„์˜ ์ง„ํ™” (์œค์„ฑ์ฒ )

    Evolution of massive stars as neutron star and black hole progenitors 1. ํ•ญ์„ฑ ์ง„ํ™”์˜ ๊ธฐ๋ณธ ์›๋ฆฌ - ๋ณ„์˜ ํ‘์ฒด ๋ณต์‚ฌ: ๋ณ„์ด ํฐ ๊ฒƒ and ๋ณ„์ด ๋œจ๊ฒ๋‹ค๋Š” ๊ฒƒ - H-R๋„ (๋Œ€๋ถ€๋ถ„์˜ ๋ณ„์ด ์ฃผ๊ณ„์—ด์„ฑ์— ์œ„์น˜ํ•˜๊ณ  ์žˆ๋‹ค, ์ดˆ๊ธฐ์—๋Š” Cooling Sequence: ํ‹€๋ฆฐ ๋ฌผ๋ฆฌ์  concept, early type, late type galaxy) - ๋ณ„์€ ์–ด๋–ป๊ฒŒ ์ง„ํ™”ํ•˜๋Š”๊ฐ€? 3๊ฐ€์ง€๋ฅผ ๊ธฐ์–ต! 1) Hydrostatic equilibrium: ์ค‘๋ ฅ๊ณผ ์••๋ ฅ์ด ์„œ๋กœ ๊ท ํ˜•์„ ๋งž์ถ”๊ณ  ์žˆ๋‹ค. ๋‹จ์œ„ ๋ณผ๋ฅจ ๋‹น ํž˜, ์••๋ ฅ ์ž์ฒด๊ฐ€ ์•„๋‹ˆ๋ผ ์••๋ ฅ์˜ gradient์™€ ๊ท ํ˜•์„ ๋งž์ถ˜๋‹ค. 2) Stars have a Negative heat capacity: ์••๋ ฅ์€ ๋‚ด๋ถ€ ์—๋„ˆ์ง€์— ๋Œ€์‘๋จ, v..

    2022.07.31
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