侲毈樇 儋膧懤艜鍒: 8 ---- 鎘樦 瀁黓罻: 0.23鼫. |
鎬賚鍻膼, 禖 羻蠈錒 瀁黓罻譔:郈-鶹請選蕭郈嚙請選蕭郈嚙請選蕭郈嚙 郈嚙請選蕭郈嚙請選蕭郈嚙踝蕭郈嚙踝蕭郈嚙 |
忺蠉鋋 僔襝鍙鍎儚殥膱 謥嚧貘鍒
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1. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect8.pdf
... 麔 侂 R 濯 蠮 v 菙 玴 6 檜 v y ) The high energy electrons will inverse-Compton ...
2. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect6.pdf
... x ∪ 1 n 擫 ~ ~ 鳵 ~ ~ " " y 鉈 Collisions 2 E=h12 1 ...
3. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect1_2.pdf
... Thus the brightness of blackbody radiation is given by 鏑 朅 g 嵕 躇 斖 燠 紿 B 膦 嵙 g 蜾 摳 邏 癲 $ ? 嵅 ? x }? ...
4. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect5.pdf
... ? ? D 鐖 D e 2 襜 鵿 鵿 睙 x { t 摳 縍 魵 q 樈 鳲 摳 俓 Radiation from A arrives at 9 6 A For semi-angle 趼 the ...
5. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect4.pdf
... Equation for emergent intensity becomes Can then estimate the mass from 鏵 P 囑 扰 e 賝 籧 皭 ~ H 淀 魵 嗖 ? 豍 樍 7 P ? 蕍 隒 鏵 P 囑 扰 e 賝 淀 Typical ...
6. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect_2.pdf
... the radiative transfer equation for a homogeneous cloud in thermal equilibrium is 爟 刷 ' B 壩 i B 壩 @ & 獿 爞 摠 1 摳 the optical depth, determines ...
7. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect3.pdf
... e.g. GHz for Orion. i G 奎 l p p 禶 At low like spectrum. ... i l W ) 熀 ( 禊 此 蘾 卑 G蘢 S q 2 城 x C ...
8. http://www.mrao.cam.ac.uk/~steve/algor2008/images/rant.pdf
... e ~ h 1z C h r q h r q h | C h d 3 f d Il 肛 r p k A 褵 5 z i A q s } C ... 8 咨 螐 嶚 q h w 9 Al p A Ip dz r z e l z 3 3 e r p 干 Cq } r Ip t 3~ 9 d ...