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3541. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.bluenearw
Mean dispersion = 1.10 angstroms / channel Start wavelength = 3412.81 angstroms End wavelength = 5389.50 angstroms Central wavelength = 4396.20 angstroms 42 lines identified from /data/maestro/bessell/sp505b Channel Wavelength Calculated Discrepancy Line # 73.7456 3491.3999 3491.4661 0.0662 1 100.5713 3520.4717 3520.5303 0.0586 2 123.7153 3545.5950 3545.6301 0.0352 3 189.9042 3617 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.bluenearw -- 4.1 Кб -- 14.06.2001
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3542. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.redcuar
CuAr red Mean dispersion = 0.54 angstroms / channel Start wavelength = 6493.12 angstroms End wavelength = 7472.03 angstroms Central wavelength = 6984.69 angstroms 32 lines identified from /data/maestro1/bessell/sp753r Channel Wavelength Calculated Discrepancy Line # 83.7305 6538.1118 6538.1655 0.0537 1 205.7369 6604.8535 6604.7686 -0.0850 2 276.9506 6643.6978 6643.7109 0.0132 3 307.9659 6660 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.redcuar -- 3.5 Кб -- 14.06.2001
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3543. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.rednearw
Coefficients of fit are - -7.65669E-09 2.32897E-05 1.08703E+00 5.54841E+03 Mean dispersion = 1.10 angstroms / channel Start wavelength = 5549.50 angstroms End wavelength = 7533.69 angstroms Central wavelength = 6538.92 angstroms 44 lines identified from /data/maestro/bessell/sp505r Channel Wavelength Calculated Discrepancy Line# 183.2512 5748.2998 5748.3462 0.0464 1 (A) 278.1969 5852.4902 5852.4580 -0.0322 2 304.9631 5881.8999 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/arlines.rednearw -- 4.3 Кб -- 14.06.2001
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3544. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/nearw.arc
... 3013.79 W 1 360 3016.47 W 1 520 3017.44 W 1 770 3024.93 W 1 210 3026.67 W 1 310 bl 3033.508 Ar 2 50 3041.73 W 1 440 bl 3043.80 W 1 270 3046.44 W 1 440 3049.69 W 1 810 3057.3907 Ne 1 300 3093.402 Ar 2 50 3093.50 W 1 370 3107.23 W 1 240 3108.02 W 1 240 3117.57 W 1 230 3120.18 W 1 260 3126.1986 Ne 1 120 3163.42 W 1 290 3176.60 W 1 320 3191.57 W 1 390 3198.84 W 1 390 3207.25 W 1 520 3215.56 W 1 1000 3243.688 Ar 2 20 3254.36 W 1 210 3259.66 W 1 210 3266.62 W 1 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/nearw.arc -- 16.7 Кб -- 14.06.2001
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3545. http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Cygnus_A.pdf
Chandra Observations of Cygnus A: Magnetic Field Strengths in the Hot Spots of a Radio Galaxy A. S. Wilson1, A. J. Young Astronomy Department, University of Maryland, College Park, MD 20742; arXiv:astro-ph/0009308 19 ... Astronomer, Space Telescope Science Institute, 3700 San Martin Drive, Balti- more, MD 21218; awilson@stsci.edu ґ2ґ ABSTRACT We report X-ray observations of the powerful radio galaxy Cygnus A with the Chandra ... We focus on the X-ray emission of the radio hotspots. ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Cygnus_A.pdf -- 109.1 Кб -- 06.05.2001
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3546. http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Pictor_A.pdf
... X-ray emission is detected from the nucleus, a 1.9 (110 kpc) long jet to the west of the nucleus, the western radio hot spot some 4.2 (240 kpc) from the nucleus, and the eastern radio lobe. ... The X-ray Emission of the Jet 4.3.1. ... Inverse Compton scattering of the synchrotron radio photons by the relativistic electrons responsible for the radio emission (i.e. a synchrotron self-Compton model) may be ruled out for the hot spot's X-ray emission, as the predicted spectrum differs from that observed...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Wilson_Pictor_A.pdf -- 324.7 Кб -- 06.05.2001
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3547. http://www.mso.anu.edu.au/pfrancis/roleplay/captain_cook1.doc
... An expedition to the South Seas would be quite expensive. ... For the same money you could build a hospital in the slums of London - a hospital that would save literally hundreds of lives a year. ... But what if the expedition discovered some new lands in the south seas? ... Why risk money on such a speculative expedition when it could be used to buy a new battleship: a very real and concrete addition to the defense of Britain. ... You are very troubled by this proposed expedition to the South Seas....
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/captain_cook1.doc -- 45.0 Кб -- 04.04.2001
[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/captain_cook1.doc -- 45.0 Кб -- 04.04.2001
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[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/captain_cook1.doc -- 45.0 Кб -- 04.04.2001
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3548. http://www.mso.anu.edu.au/~geoff/HEA/Perley.pdf
... The radio structure is found to comprise very dim, nearly circular lobes with an extraordinarily bright and compact hot spot located at the western extremity of the western lobe. ... Further, the extraordinary brightness ratio between the western hot spot and the unusually dim and circular lobes argues for some unusual differences between this object and more `normal' examples of radio-loud AGN. ... Fig. ... The lobes Fig. 3 shows Pictor A at 20 cm with a resolution of 10 . ... A similar fea- Fig. ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Perley.pdf -- 2005.0 Кб -- 20.03.2001
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3549. http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf
... Frequently the environments in which this emission occurs are created by High Energy Astrophysics : Overview 3/47 the transfer of prodigious amounts of energy and momentum. e.g. Ї Accretion onto black holes Ї Transfer of energy and momentum via jets Ї Processing of the interstellar medium via blast waves whose ultimate source of energy is prodigious e.g. the explosion of a star Ї Heating of the interstellar medium of a ... 5.Radio emission from radio galaxies and quasars. ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf -- 2636.4 Кб -- 04.03.2001
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3550. http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/readme_Aperplates
... Q 12.649 0.523 0.342 -0.108 4444 -4.647 -4.582 "n6231_ 178" 16 53 48.63 -41 51 54.1 J2000.0 ! ... A few lines are then added to the top (see readme_asc2dxf for details) to produce input for asc2dxf :in.coo: n6231cp6.dxf slot line 2.00 43.00 9.00 43.00 point 9.773 19.026 n6231 _ 171 Q 12.649 11.236 57.382 n6231 _ 178 I 14.533 ... the output of this program is as follows :n6231cp6.dxf: 0 SECTION 2 ENTITIES 0 CIRCLE 8 1 62 3 10 43.00 20 43.00 30 0.000 40 43.00 0 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/readme_Aperplates -- 3.0 Кб -- 14.02.2001
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3551. http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/readme_asc2dxf
... Once "point" is read, assumes all the following x,y coordinates are points. ... Program asc2dxf c reads set of x,y coordinates and writes a .dxf file for aperture plate. character*4 xop1,xop2 character*12 outfile 1 format ( 1h0 /7hSECTION/1h2/8hENTITIES/ 1h0 ) 2 format (6hCIRCLE/1h8/1h1/2h62/1h3) 3 format (4hLINE/1h8/1h1/2h62/1h3) 4 format (5hPOINT/1h8/1h1/2h62/1h3) 5 format (2h10/5h43.00/2h20/5h43.00/2h30/5h0.000/2h40/5h43.00/ 1h0 ) 6 format (2h10,/,f6.3,/,2h20,/,f6.3,/,2h30/5h0.000) 7 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/readme_asc2dxf -- 4.7 Кб -- 14.02.2001
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3552. http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/n6705cp6m13.8.in
n6705cp6m13.dxf noslot point 12.567 47.669 m11_6274 13.572 17.079 64.434 m11_6446 13.896 19.195 35.114 m11_6519 13.951 19.812 67.240 m11_6541 13.771 24 ... ; 13.862 30.203 72.949 m11_6944 13.892 30.638 38.029 m11_6963 13.967 32.815 59.100 m11_7056 13.631 34.303 56.257 m11_7119 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Workshop/applic/n6705cp6m13.8.in -- 2.3 Кб -- 14.02.2001
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3553. Users Guide
... This autoguider system consists of an Apogee direct CCD Camera that views part of the DBS slit via Focal Reducer Optics, and a PC computer running MaxIm CCD Camera Control and Image Processing Software. ... Pulling a star into the slit. ... New - Guiding aperture plates. ... The focus tab in the MaxIm CCD window allows user or auto selection of a subframe for telescope focussing. ... Get used to using the left image window with the expose tab and the right image window with the guide tab. ...
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Ссылки http://www.mso.anu.edu.au/~conroy/DBS-Autoguider-Manual/dbs-autoguider-v3.htm -- 27.4 Кб -- 06.12.2000
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3554. http://www.mso.anu.edu.au/pfrancis/roleplay/roleplay_action_research_writeup/outlinec.htm
A study of Role-playing Games in Undergraduate Astronomy Classes . ... Classroom Role-playing Games . PPT Slide . ... Minute Papers . ... How many students mentioned, in their minute papers, that the most important thing they had learned that week was about the nature of science? Minute paper responses . Typical quotes: УThe most important thing I learned this week wasЕФ . ... ANUSET Questionnaire Responses . ... More quotes . ... More Detailed Conclusions. Conclusions . ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/roleplay_action_research_writeup/outlinec.htm -- 3.3 Кб -- 18.10.2000
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/roleplay_action_research_writeup/outlinec.htm -- 3.3 Кб -- 18.10.2000
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/roleplay_action_research_writeup/outlinec.htm -- 3.3 Кб -- 18.10.2000
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3555. A study of Role-playing Games in Undergraduate Astronomy Classes
Your browser does not support frames. Try Internet Explorer 3.0 or later or Netscape Navigator 2.0 or later .
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/roleplay_action_research_writeup/ppframe.htm -- 5.5 Кб -- 18.10.2000
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/roleplay_action_research_writeup/ppframe.htm -- 5.5 Кб -- 18.10.2000
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/roleplay_action_research_writeup/ppframe.htm -- 5.5 Кб -- 18.10.2000
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3556. A study of Role-playing Games in Undergraduate Astronomy Classes
A study of Role-playing Games in Undergraduate Astronomy Classes . ... Classroom Role-playing Games . PPT Slide . ... Minute Papers . ... How many students mentioned, in their minute papers, that the most important thing they had learned that week was about the nature of science? Minute paper responses . ... More Detailed Conclusions. Conclusions . ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/roleplay_action_research_writeup/ -- 3.2 Кб -- 18.10.2000
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/roleplay_action_research_writeup/index.htm -- 3.2 Кб -- 18.10.2000
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/roleplay_action_research_writeup/ -- 3.2 Кб -- 18.10.2000
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/roleplay_action_research_writeup/index.htm -- 3.2 Кб -- 18.10.2000
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/roleplay/roleplay_action_research_writeup/ -- 3.2 Кб -- 18.10.2000
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3557. http://www.mso.anu.edu.au/~geoff/AGD/Relativistic_Applications.pdf
... Relativistic Applications 4/14 2 Superluminal motion 2.1 Apparent transverse velocity P 1 V l = Vt P 2 To d = V t cos l = V t sin observer D Consider an object which moves from P 1 to be emitted from P 1 and P 2 at times t 1 and P 2 in a time t in the observer's frame. ... Relativistic Applications 8/14 3 Speed of advance of a hotspot Terminal shock This picture represents the generic sitjet uation of jet forcing it way through the interstellar medium. ... Relativistic Applications 14/14 ...
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Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Relativistic_Applications.pdf -- 222.7 Кб -- 29.08.2000
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3558. Pink Black Holes ? the Real Story
... This is the story of pink black holes, and how they were discovered. ... The first quasars were discovered early in the 1960s, using radio telescopes. ... In some bizarre way, these black holes were devouring the gas and stars around them, and spitting some of the debris out at nearly the speed of light in two powerful jets. ... He noticed that most quasars looked extremely blue when observed with an optical telescope. ... Why should black holes be incredibly blue? ... So, many quasars are pink. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/pink/true_story.htm -- 17.8 Кб -- 21.08.2000
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/pink/true_story.htm -- 17.8 Кб -- 21.08.2000
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~pfrancis/pink/true_story.htm -- 17.8 Кб -- 21.08.2000
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3559. http://www.mso.anu.edu.au/~geoff/HEA/bdo.pdf
... Printed in U.S.A. UNIFICATION OF THE RADIO AND OPTICAL PROPERTIES OF GIGAHERTZ PEAK SPECTRUM AND COMPACT STEEP-SPECTRUM RADIO SOURCES GEOFFREY V. BICKNELL,1 MICHAEL A. DOPITA,2 AND CHRISTOPHER P. O. OоDEA3 Received 1996 October 2 ; accepted 1997 February 7 ABSTRACT We adopt the view that the classes of active galactic nuclei (AGN) known variously as gigahertz peak spectrum (GPS) sources , compact steep-spectrum ( CSS ) ... However, studies of the radio spectra of CSS sources (Fanti et al....
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/bdo.pdf -- 1512.1 Кб -- 31.05.2000
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3560. http://www.mso.anu.edu.au/~geoff/HEA/mundell.pdf
... Parsec-Scale Images of Flat-Spectrum Radio Sources in Seyfert Galaxies C.G. Mundell Department of Astronomy, University of Maryland, College Park, MD, 20742, USA; A.S. Wilson1 ... Department of Astronomy, University of Maryland, College Park, MD, 20742, USA; astro-ph/9908255 23 Aug 1999 J.S. Ulvestad National Radio Astronomy Observatory, P.O. Box O, Socorro, NM, 87801,USA; A.L. Roy2 National ... 1998; Taylor et al., ... 1998. ... The 8.4-GHz VLBA image Figure 1 shows an unresolved source. ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/mundell.pdf -- 623.9 Кб -- 31.05.2000
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