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3201. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l1788.tab
... Telluric lines removed by Bessell set .z.units = micro-Janskys set .z.label = Flux set .table.bandwidth = 50 * 3300 6522 3350 6906 3400 7119 3450 7191 3500 7406 3550 7900 3600 8279 3650 8774 3700 8937 3750 9350 3800 10510 3850 11036 3900 11251 3950 11056 4000 12717 4050 13292 4100 12978 4150 13880 4200 13983 4250 14164 4300 14151 4350 13919 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l1788.tab -- 3.0 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l1788.tab -- 3.0 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l1788.tab -- 3.0 Кб -- 23.11.2008
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3202. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l7379.tab
... Telluric lines removed by Bessell set .z.units = micro-Janskys set .z.label = Flux set .table.bandwidth = 50 * 3300 66069 3350 66009 3400 72244 3450 72711 3500 77339 3550 83253 3600 81658 3650 94102 3700 98537 3750 96472 3800 109749 3850 105390 3900 111892 3950 96205 4000 147231 4050 161287 4100 165806 4150 177011 4200 175711 4250 170765 4300 157471 4350 179473 4400 190195 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l7379.tab -- 3.2 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l7379.tab -- 3.2 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l7379.tab -- 3.2 Кб -- 23.11.2008
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3203. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l9491.tab
... Telluric lines removed by Bessell set .z.units = micro-Janskys set .z.label = Flux set .table.bandwidth = 50 * 3300 8340.648 3350 8637.736 3400 8677.608 3450 8503.540 3500 8637.736 3550 8733.735 3600 8847.081 3650 8961.897 3700 8961.897 3750 8978.419 3800 8994.971 3850 9069.851 3900 8961.897 3950 9028.176 4000 8994.971 4050 9179.094 4100 9136.922 4150 9078.204 4200 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l9491.tab -- 4.5 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l9491.tab -- 4.5 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/ltt9491.tab -- 4.5 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l9491.tab -- 4.5 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/ltt9491.tab -- 4.5 Кб -- 23.11.2008
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3204. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/lpoext.tab
... T A B * * Extinction table for LPO. ... SET .Z.LABEL = Extinction * 3000 3.7150 3100 1.5961 3200 0.9908 3300 0.6967 3400 0.5934 3500 0.5146 3600 0.4554 3700 0.4061 3800 0.3633 3900 0.3260 ... 9200 0.0099 9300 0.0095 9400 0.0091 9500 0.0087 9600 0.0083 9700 0.0080 9800 0.0077 9900 0.0074 10000 0.0071 10100 0.0068 10200 0.0065 10300 0.0063 10400 0.0060 10500 0.0058 10600 0.0056 10700 0.0054 10800 0.0052 10900 0.0050 11000 0.0048 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/lpoext.tab -- 2.6 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/lpoext.tab -- 2.6 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/lpoext.tab -- 2.6 Кб -- 23.11.2008
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3205. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/one.tab
one * * Dummy set .z.units = micro-Janskys set .z.label = Flux set .table.bandwidth = 50 * 3200 1 3250 1 3300 1 3350 1 3400 1 3450 1 3500 1 3550 1 3600 1 3650 1 3700 1 3750 1 3800 1 3850 1 3900 1 ... 1 9100 1 9150 1 9200 1 9250 1 9300 1 9350 1 9400 1 9450 1 9500 1 9550 1 9600 1 9650 1 9700 1 9750 1 9800 1 9850 1 9900 1 9950 1 10000 1 10050 1 10100 1 10150 1 10200 1 10250 1 10300 1 10350 1 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/one.tab -- 3.6 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/one.tab -- 3.6 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/one.tab -- 3.6 Кб -- 23.11.2008
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3206. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/aaoext.tab
... T A B * * Extinction table for AAO. ... SET .Z.LABEL = "Extinction" * 3200 1.084 3250 0.948 3300 0.858 3350 0.794 3400 0.745 3450 0.702 3500 0.665 3571 0.617 3636 0.575 3704 0.532 3862 0.460 4036 0.396 4167 0.352 4255 0.325 4464 0.279 4566 0.259 4785 0.234 5000 0.203 5263 0.188 5556 0.177 5840 0.166 6056 0.160 6436 0.123 6790 0.098 7100 0.094 7550 0.080 7780 0.076 8090 0.080 8370 0.077 8708 0.057 9832 0.080 10256 0.050 10400 0.051 10610 0.053 10796 0.056 10870 0.064 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/aaoext.tab -- 1.8 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/aaoext.tab -- 1.8 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/aaoext.tab -- 1.8 Кб -- 23.11.2008
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3207. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/extin.tab
* * Mean Extinction Coefficients for Palomar Mountain * * from Hayes & Latham 1975, Ap.J. 197, p597 * 3200 1.058 3250 0.911 3300 0.826 3350 0.757 3390 0.719 3448 0.663 3509 0.617 3571 0.575 3636 0.537 3704 0.500 3862 0.428 4036 0.364 4167 0.325 4255 0.302 4464 0.256 4566 0.238 4785 0.206 5000 0.183 5263 0.164 5556 0.151 5840 0.140 6055 0.133 6435 0.104 6790 0.084 7100 0.071 7550 0.061 7780 0.055 8090 0.051 8370 0.048 8708 0.044 9832 0.036 10255 0.034 10610 0.032 10795 0.032 10870 0.031
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/extin.tab -- 1.6 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/extin.tab -- 1.6 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/palobsextin.tab -- 1.6 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/extin.tab -- 1.6 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/palobsextin.tab -- 1.6 Кб -- 23.11.2008
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3208. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/extinaao.tab
Mean Extinction Coefficients for AAO * 3000 1.415 3050 1.415 3100 1.415 3150 1.41 3200 1.093 3250 0.946 3300 0.860 3350 0.791 3390 0.753 3420 0.725 3448 0.697 3509 0.650 3571 0.608 3636 0.570 3704 0.532 ... .190 5556 0.176 5630 0.173 5698 0.170 5840 0.164 5948 0.160 6055 0.156 6143 0.149 6231 0.141 6435 0.126 6790 0.106 7100 0.092 7550 0.081 7780 0.075 8090 0.071 8370 0.068 8708 0.063 9832 0.056 10255 0.054 10400 0.052 10610 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/extinaao.tab -- 1.7 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/extinaao.tab -- 1.7 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/extinaao.tab -- 1.7 Кб -- 23.11.2008
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3209. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/extinsso.tab
... T A B * * Extinction table for AAO. ... Based on Hayes and Latham. * set .z.label = "Extinction" * 3200 1.093 3250 0.946 3300 0.860 3350 0.791 3390 0.753 3448 0.697 3509 0.650 3571 0.608 3636 0.570 3704 0.532 3862 0.460 4036 0.395 4167 0.355 4255 0.332 4464 0.285 4566 0.266 4785 0.234 5000 0.210 5263 0.190 5556 0.176 5840 0.164 6055 0.156 6435 0.126 6790 0.106 7100 0.092 7550 0.081 7780 0.075 8090 0.071 8370 0.068 8708 0.063 9832 0.056 10255 0.054 10400 0.052 10610 0.053 10795 0.053 10870 0.052 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/extinsso.tab -- 1.6 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/extinsso.tab -- 1.6 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/extinsso.tab -- 1.6 Кб -- 23.11.2008
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3210. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/f110.tab
F110 Hamuy * set .z.units = Ergs/s/cm**2/A set .z.label = Flux set .table.bandwidth = 50 * 3300.00 6.743e-13 3350.00 6.604e-13 3400.00 6.236e-13 3450.00 5.757e-13 3500.00 5.487e-13 3550.00 5.260e ... .00 1.472e-13 5150.00 1.426e-13 5200.00 1.381e-13 5250.00 1.329e-13 5300.00 1.280e-13 5350.00 1.242e-13 5400.00 1.178e-13 5450.00 1.156e-13 5500.00 1.119e-13 5550.00 1.082e-13 5600.00 1.043e-13 5650.00 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/f110.tab -- 3.7 Кб -- 23.11.2008
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/f110.tab -- 3.7 Кб -- 23.11.2008
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/f110.tab -- 3.7 Кб -- 23.11.2008
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3211. http://www.mso.anu.edu.au/~charley/papers/SullivanBaross.pdf
BOOK REVIEWS 607 attention and students. ... With the publication of Planets and Life, a textbook for graduate students and upper level undergraduates, astrobiology is taking another large step towards formalizing itself as an established multidisciplinary field. ... This book combines reviews of existing evidence for mantle plumes with the results from recent studies and uses them to understand the upper mantle structure beneath several of the world's volcanic regions. ... Planets and Life. ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/SullivanBaross.pdf -- 35.1 Кб -- 20.11.2008
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3212. http://www.mso.anu.edu.au/~brian/A3002/probset2-2008.pdf
Problem Set 2 - CosmologyґA3002 ґDue on or before November 7th. Can be sent via internal mail (Brian Schmidt, RSAA) use H0=70 km/s/Mpc, M=0.27, =0.73, w=-1 for all problems. ... Finish off your Monte Carlo simulation by selecting objects at random redshifts from 0<z<0.1, assuming that they have a mean absolute magnitude of M=-19.5 with a dispersion 0.2 magnitudes. ... Problem 2.1 (2 pt): In class we described the scale at which material can collapse in the Universe as the Jeans' length. ...
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Ссылки http://www.mso.anu.edu.au/~brian/A3002/probset2-2008.pdf -- 86.1 Кб -- 27.10.2008
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3213. http://www.mso.anu.edu.au/~brian/A3002/lecture1_last_a.pdf
... It is common to use the shorthand of Galactic quadrants when discussing directions of the Galaxy: First Quadrant: 0 l 90o Second Quadrant: 90o l 180o Third Quadrant: 180o l 270o Fourth Quadrant: 270o l 360o 13 Galactic Coordinates (cont.) l = 0 - Galactic center l = 90 - in the direction of Galactic rotation l = 180 - anticenter l = 270 - antirotation III II www.thinkastronomy.com IV I l = 0 - 90 l = 90 - 180 first quadrant second ...
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Ссылки http://www.mso.anu.edu.au/~brian/A3002/lecture1_last_a.pdf -- 920.8 Кб -- 15.09.2008
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3214. http://www.mso.anu.edu.au/~brian/A3002/Assignment_Carollo.pdf
... You can also send a pdf version by email to carollo@mso.anu.edu.au The structures and star populations in the Milky Way [12 points ] Daniela Carollo ґ 09/09/08 ґ 12/09/08 ASSIGNMENTS Problem N. 1 a. (1 point) Using the formula of the propagation errors demonstrate the following relation (Lecture N. 1): d/d = /. b. (2 points ) Also, given the following spectral type: Main Sequence: Giants: F5 G0 M0 K5 M0 for a given limit magnitude of the telescope mV = 20, ...
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Ссылки http://www.mso.anu.edu.au/~brian/A3002/Assignment_Carollo.pdf -- 168.9 Кб -- 15.09.2008
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3215. http://www.mso.anu.edu.au/~brian/A3002/grtinypdf.pdf
... This naturally leads to a view in which space and time are joined together to form spacetime; the conversion factor from time units to space units is c (which equals 1, right? couldn't be simpler). ... Note a few things: these indices are superscripts, not exponents. ... The x? are coordinates on this manifold. ... The Minkowski metric is of course just the spacetime generalization of the ordinary inner product on flat Euclidean space, which we can think of in components as the Kronecker delta, ij ....
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Ссылки http://www.mso.anu.edu.au/~brian/A3002/grtinypdf.pdf -- 175.3 Кб -- 04.09.2008
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3216. http://www.mso.anu.edu.au/~kcf/ATA/pan_spectr.pdf
... New high resolution multi-ob ject spectrographs on 4-8m class telescopes (HERMES, WFMOS) will allow us for the first time to make large and detailed chemical abundance surveys of stars in the Galactic disk, bulge and halo, and apply the techniques of chemical tagging to recovering the fossil information left over from galaxy assembly. ... Conclusion The ultimate goal of the prop osed WFMOS high resolution survey is unravelling the star formation history of the disk and halo via chemical tagging. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/ATA/pan_spectr.pdf -- 76.8 Кб -- 12.08.2008
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3217. http://www.mso.anu.edu.au/~bessell/FTP/EpsCha_spectra/EpsCha_Normalised_Spectra.txt
wavelength Eps ChaAB HD104237AC HD104237E 2MASS J12014343 HD104237D 2MASS J12074598 CXOU J115908.2 CXOU J120152.8 USNO B120144.7 2MASS J12005517 3500.0 5.02517e-01 3.78219e-01 2.93927e-02 1.38979e-01 1.09065e-01 4.02655e-02 8.67989e-03 1.78412e-02 1.29572e-02 2.19594e-02 3504.0 5.23406e-01 4.03979e-01 3.00139e-02 1.40516e-01 1.10674e-01 2.80250e-02 2.67481e-03 3.21887e-03 -4.75818e-03 -2.96531e-02 3508.0 5.10553e-01 4.05967e-01 3.08239e-02 -5.65817e-02 1.02318e-01 3.45119e-02 1.56196e-02 -1.57067e-03
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/EpsCha_spectra/EpsCha_Normalised_Spectra.txt -- 210.8 Кб -- 03.07.2008
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3218. http://www.mso.anu.edu.au/~charley/papers/RoblesLineweaverAstroph.pdf
A comprehensive comparison of the Sun to other stars: searching for self-selection effects JosЄ A. Robles1 , Charles H. Lineweaver1 , Daniel Grether2 , Chris Flynn3 , Chas A. Egan2,4 , e Michael B. Pracy4 , Johan Holmberg5 and Esko Gardner3 arXiv:0805.2962v1 [astro-ph] 19 May 2008 ABSTRACT If the origin of life and the evolution of observers on a planet is favoured by atypical prop erties of a planet's host star, we would exp ect our Sun to b e atypical with resp ect to such prop erties. ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/RoblesLineweaverAstroph.pdf -- 2242.0 Кб -- 20.05.2008
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3219. http://www.mso.anu.edu.au/~akarakas/Kodai_Lecture2.pdf
... Introduction to AGB stars, and the evolution prior to the AGB phase 2. ... Evolution and nucleosynthesis of AGB stars 4. ... Super-AGB stars and post-AGB objects Outline of this lecture 1. ... V a lu e s d i ff e r e n t f o r s h e ll b u r n i n g b e c a u s e h i g h e r T Non-energetic reactions Ї He-burning occurs in the ashes of H- burning Ї Composition is 98% 4He, ~2% 14N Ї Nitrogen-14 can capture alpha particles to produce secondary nuclei, depending on T: ґ ґ 14N ...
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Ссылки http://www.mso.anu.edu.au/~akarakas/Kodai_Lecture2.pdf -- 2614.8 Кб -- 10.05.2008
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3220. http://www.mso.anu.edu.au/~charley/papers/NormanLineweaver2008.pdf
New Perspectives on the Lunar Cataclysm from Pre-4 Ga Impact Melt Breccia and Cratering Density Populations Marc Norman1,2 and Charles H. Lineweaver1 1 Planetary Science Institute of the Research ... Earth Sciences and the Research School of Astronomy and Astrophysics, Australian National University, Canberra ACT 0200 Australia 2 Lunar and Planetary Science Institute, 3600 Bay Area Boulevard, Houston TX 77058 USA Abstract Crystallisation ages of impact ... Was There a Late Cataclysm? ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/NormanLineweaver2008.pdf -- 604.5 Кб -- 07.05.2008
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