侲毈樇 儋膧懤艜鍒: 8 ---- 鎘樦 瀁黓罻: 0.21鼫. |
鎬賚鍻膼, 禖 羻蠈錒 瀁黓罻譔:-鶹踝蕭嚙踝蕭嚙請選蕭郈嚙請選蕭郈嚙請選蕭郈嚙請選蕭郈嚙請選蕭郈嚙 郈嚙踝蕭郈嚙踝蕭郈嚙踝蕭郈嚙踝蕭郈嚙踝蕭郈嚙踝蕭郈嚙踝蕭郈嚙踝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 ...