Ralph Sutherland RSAA, ANU, ANITA Cooling in the ISM Cooling in the ISM Example: Nearby RGs with Resolved Hosts M87 Sparkes et al 2004 astro-ph/0402204 Example: Active Galaxies: Cen A Example: Equilibrium Heating and Cooling : HII regions Example: Galactic ISM Example: Galactic ISM Example: z= 3.8 galaxy 4C41.7 4C41.17 Scharf et al 2003 Theoretical Approach: ISM thermal emission -12.0 II III I 0.0 -1.0 12.0 11.0 10.0 9.0 rec. eq. cool p r e IV V,VI -2.0 -3.0 -4.0 coll. cool eq. ...

... For example, the previous examples are periodic. Example Dual beam calibration observation of a strong-point source with the GBT: Example Dual beam calibration observation of a strong-point source with the GBT: 0 -1 -2 Tb -3 -4 0 1000 2000 3000 t 4000 5000 6000 Example 1/f spectrum Shor t section of the data away from the strong source Time stream Power spectral density -1.75 -1.76 -1.77 -1.78 -1.79 240 260 280 300 t 320 340 360 15 5 5 15 25 0.0 0.2 0.4 Frequency 0.6 Power ...

... Nonparametric density estimation drops these restrictions 8 Nonparametric Density Estimation 12 density 0 0.0 2 4 6 8 10 0.1 0.2 0.3 redshift 0.4 0.5 Histogram of 1,425 galaxy redshifts. 9 Nonparametric Density Estimation 12 density 0 0.0 2 4 6 8 10 0.1 0.2 0.3 redshift 0.4 0.5 Compared with best fitting gamma distribution. ... 13 Nonparametric Density Estimation 12 density 0 0.0 2 4 6 8 10 0.1 0.2 0.3 redshift 0.4 0.5 Parametric versus nonparametric estimate (kernel density estimate). ...

Declination: -85.0 -80.0 -75.0 -70.0 -65.0 -60.0 -55.0 -50.0 -45.0 -40.0 -35.0 -30.0 - 25.0 - 20.0 - 15.0 - 10.0 - 5.0 0.0 5.0 10.0 15.0 20.0 25.0 degrees Wavelength: 3800.0 3900.0 4000.0 4100.0 4200.0 4300.0 4400.0 4500.0 4600.0 4700.0 4800.0 4900.0 5000.0 5100.0 5200.0 5300 ASCII file: . PDF file: . PNG file: . ...

from __future__ import division from visual import * scene = display(range=(3.0,3.0,3.0),width=1300,height=800,forward=( 0.2 ,-0.3,-1.0)) water = box( pos =(0,- 0.1 , 0.0 ), length=10, width=3, height= 0.1 , color =( 0.1 , 0.2 ,1.0)) alength = 2.0 theta = 0.1 pos1 = vector (0,0,0.6) barge1 = box( pos = pos1, length = 2, width = 0.5, height = 0.1 , color =(0.6,0.4, 0.2 )) x1 = arrow( pos = pos1+ vector (0, 0.1 ,0), ...

... OH, = 18 cm Nancay Radio Telescope, OH 18-cm line observations , since 1969 F, Jy 6 4 2 0 0 -1 -2 0 -1 -2 0 -2 -4 -6 30 40 50 1612 MHz I HU Pup August 5, 2009 1665 MHz 4 2 0 0.5 0.0 - 0.5 -1.0 -1.5 1.0 0.5 0.0 - 0.5 4 3 2 1 0 -1 1667 MHz I I 1.0 0.5 0.0 0.5 0.0 22-meter telescope, Pushchino Radio Astronomy Observatory H2O F, Jy 1.0 0.5 0.0 0.4 0.2 0.0 -0.2 -0.4 0.4 0.2 0.0 -0.2 -0.4 -0.6 0.6 0.4 0.2 0.0 -0.2 -0.4 -70 -60 -50 -40 -30 -20 -10 0 Mira-type star R Leo. ...

... ФЭУ; 6. усилитель; 7. крейт; 8. вольтметр; 9. блок управления шаговым двигателем; 10. крейт-контроллер; 11. редуктор; 12. шаговый двигатель; 13. персональный компьютер; 14. блок питания ФЭУ; 15. блок питания усилителя и шагового двигателя 0 500 1000 1500 2000 2500 3000 3500 3500 4000 4500 5000 5500 6000 6500 7000 7500 8000 Wavelength, A O 2 H 2 O O 2 Спектр Солнца. ... 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 3500 4000 4500 5000 5500 6000 6500 Wavelength, A Ha Na Hg Hb Mg Эквивалентный спектр поглощения. ...

filter wavelength Calculated V1 Calculated V2 Abs Wave ; ------ ---------- ------------- ------------- -------- S I r 1 3 -1.5298 -639.0000 -662.0000 6561.5000 3 -1.2287 -420.0000 - 599.0000 6561.8000 3 -1.0279 -274.0000 -557.0000 6562.0000 3 -0.8272 -128.0000 -515.0000 6562.2000 3 -0.6264 18.0000 -473.0000 6562.4000 3 - 0.4298 161.0000 -432.0000 6562.6000 3 - 0.3294 234.0000 -411.0000 6562.7000 3 - 0.2291 307.0000 -390.0000 6562.8000 3 - ...

` . Minor Planets sorted by names .

Impact ­ Produced Exosphere of Europa A.A. Berezhnoy Sternberg Astronomical Institute, Moscow, Russia Equilibrium chemical composition of the impact-induced cloud 0.5 0.45 0.4 0.35 0.3 0.25 0.2 0.15 0.1 3000 3500 4000 T, K 4500 OH H2 5000 O 5500 H H2O Q 0.0045 0.004 0.0035 0.003 0.0025 0.002 0.0015 0.001 0.0005 0 2000 Na NaO H NaO 3000 T, K 4000 5000 1.E-01 2000 Q 1.E-02 1.E-03 1.E-04 T, K 2500 CO 3000 ... Previous detection of cometary impacts on Europa is very tentative. ...

... Sum in visible - 500 k R . ... 16.4 nsec . ... Auroral, . ... 0.2 . ... Sum - 10-100 . 250 . ... Sum - 20-400 . ... sum –500 . ... Sum - <10R . ...

Motivation Long-term precession Relativistic Effects Conclusions . ... for long time interval Kai Tang, Michael H. Soffel, Jin-He Tao, Zheng-Hong Tang 2014-09-22 St. Petersburg () Journess2014 2014-09-22 1 / 19 Motivation Long-term precession Relativistic Effects Conclusions . ... 2 Long-term precession . ... 4 Conclusions St. Petersburg () Journess2014 2014-09-22 2 / 19 Motivation Long-term precession Relativistic Effects Conclusions Contents . ... St. Petersburg () Journess2014 2014-09-22 19 / 19 ...

. Mg x Fe 1-x O from Henning et al. (1995) . Use our codes to transform the standard data file to another form. Back to paper page . Last modified: 25/09/98, V.I.

Change in Brightness Kepler 4b 0.0 % - 0.1 %0.12 - 0.2 % 0.14 0.16 0.18 0.02 0.04 0.06 0.08 Transit Light Curves Set 1 Transit Tracks p. 3 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-7b 0.0 % -1.0% -2.0% 0.2 0.4 0.6 0.8 1.2 1.4 1.6 1.8 2.2 2.4 2.6 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-11b 0.0 % -0.5% -1.0% ...

Rfmonitor data:100401 .5*(maxAllowable exposure) 1.6 1.4 1.2 1.0 0.8 0.6 0.4 0.2 5 10 15 Hour of day Ast 20 Rfmonitor data:100701 .5*(maxAllowable exposure) 1.6 1.4 1.2 1.0 0.8 0.6 0.4 0.2 5 10 15 Hour of day Ast 20 Rfmonitor data:100801 .5*(maxAllowable exposure) 1.0 0.5 0.0 -0.5 -1.0 -1.5 5 10 15 Hour of day Ast 20 Rfmonitor data:101001 .5*(maxAllowable exposure) 4.10 4.05 4.00 3.95 3.90 5 10 15 Hour of day Ast 20

... Armagh Observatory 2001 July */ #declare Shining_Dwarf_Core = sphere{ 0,0,0 , 0.99 hollow on interior{ media{ absorption rgb 0.0 , 0.0 , 0.0 scattering { 5 rgb 1.0 , 1.0 , 1.0 eccentricity + 0.1 } density { spherical color_map{ [0.00 rgb 0,0,0 ] [ 0.05 rgb 0.1 , 0.1 , 0.5 ] [ 0.2 rgb 0.2 , 0.2 , 0.6 ] [ 0.5 rgb ...

DIMM . ... 100 000 , 2007 ­ 2009 . ... S 0.2). ... 1 3 ) , D DIMM. s DIMM s= D r0 5/3 = 5 D 2 · l2,t , Kl,t (1 4 ) 1.0 S a 0.9 0.8 0.7 LE MTF SE MTF S a 0.6 0.5 0.4 0.3 0.2 0 1 2 3 4 5 6 5/3 7 8 9 10 s = (D/r0) . ... Smin > 0.45, Smin < 0.45, - DIMM, 7 - 8 . ... Smin > 0.45 ( ) Smin < 0.45 , . ... Smin > 0.3 7 l / 0.8 0.6 S o t 1.0 0.4 0.2 Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep 2008 2009 . ... 8 MASS/DIMM 2007 2009 , , , , . ...

Сатурн в 2007 году: . ... Максимальный блеск: -0.0m - февраль 2007 . ... Склонение РдС РдЗ mag Элонг.Созв. -------------------------------------------------------------------- 1 янв 09h48m17.57s +14њ32' 14.8 9.178 8.4483 0.2 135.7 Leo 11 янв 09h46m15.15s +14 44' 39.1 9.180 8.3446 0.2 146.4 Leo 21 янв 09h43m41.98s +14 59' 22.0 9.182 8.2668 0.1 157.3 Leo 31 янв 09h40m46.49s +15 15' 33.6 9.185 8.2182 0.0 168.2 Leo 10 фев 09h37m38.64s +15 32' 18.3 9.187 8.2004 - ...

... 4 3000 3500 4000 4500 5000 5500 6000 6500 7000 7500 8000 8500 9000 Tarusa 19.01.2012 - p. 9 Time dependent at 15 Day 1.8з10 14 15 day H, CA time dep endent f (er g /s/cm2/H z ) 0. ... 6 3000 3500 4000 4500 5000 5500 6000 6500 7000 7500 8000 8500 9000 Tarusa 19.01.2012 - p. 10 Steady state, time dependent at 15 Day 1.8з10 14 15 day H, CA time dep endent steady state f (er g /s/cm2/H z ) 0. ... 2 3000 3500 4000 4500 5000 5500 6000 6500 7000 7500 8000 8500 9000 Tarusa 19.01.2012 - p. 21 ...

... INTRODUCTION A detailed analysis of high-accuracy, multi-color light curves of the binary system with an exoplanet HD 209458 [1] demonstrated a discrepancy between the observed limb-darkening coefficients and theoretical values obtained from model stellar atmospheres. ... CONCLUSION We have analyzed multi-color transit light curves of the star­exoplanet binary systems HD 209458 and HD 189733 using the theoretical limb-darkening coefficients of [15] and a quadratic limb-darkening law. ...