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3221. http://www.mso.anu.edu.au/~chiaki/works/TEN80301.pdf
... WMAP Q Q Q CDM QQ Q QQ Q Q Q QQ Q Q QQ Q QQ Q Q Q Q 101 Q Q Q Q Q QQ QQ Q Q Q Q Q Q Q Q Q QQ Q 4), 5) QQ QQ QQ Q Q QQ Q QQQQQ QQQ Q QQ Q Q QQ QQQQ QQQQ Q QQ QQ Q Q Q Q QQ QQ Q Q QQ QQ Q Q Q Q Q Q QQQQ Q Q Q Q QQQ Q QQQQ Q QQQQ Q QQ Q QQQ QQQQ Q QQQ Q Q Q Q Q Q Q Q Q Run Q QQ 2) 1) Millennium 100 Q QQ QQ Q QQ Q Q 3) QQ QQQ Q 500 Mpc N QQ Q Q Q QQ QQ Q Q 90 QQ Q Q QQ Q QQ Q QQ QQ Q QQQ QQ QQQQ QQQ ...
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Ссылки http://www.mso.anu.edu.au/~chiaki/works/TEN80301.pdf -- 2146.0 Кб -- 08.02.2008
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3222. http://www.mso.anu.edu.au/~charley/papers/ReplytoFlambaum2003.pdf
AST ROB IOL OG Y Vol um e 3 , Nu mb er 2 , 20 0 3 ? Ma ry Ann Lie b ert, In c. Rapid Communication On the Nonobservability of Recent Biogenesis CHARLES H. LINEWEAVER1,2 and TAMARA M. DAVIS1 I "Does the rapid appearance of life on Earth suggest that life is common in the Universe?" ... In the accompanying comment Flambaum (2003) argues that there are "a large number of crucial intermediate steps between the first live organisms and humans." These steps take a long time. ... The Sun is 4.56 Gyr old. ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/ReplytoFlambaum2003.pdf -- 100.7 Кб -- 30.01.2008
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3223. http://www.mso.anu.edu.au/~raquel/Disk06poster.pdf
Angular Momentum Transport in Protoplanetary Disks Raquel Salmeron(1), Arieh KЖnigl ( 1) Mark Wardle ( 2) ( 1 ) D e p t. A s tr o n o m y A s tr o p h y s ic s , U n iv e r s ity o f C h ic a g o ( 2 ) D e p t. P h y s ic s , M a c q u a r ie U n iv e r s ity Abstract Angular momentum (l ) transport in protostellar disks can take place either radially, through turbulence induced by the magnetorotational instability (MRI), or ... It measures the magnetic field strength. ...
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Ссылки http://www.mso.anu.edu.au/~raquel/Disk06poster.pdf -- 695.0 Кб -- 07.01.2008
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3224. http://www.mso.anu.edu.au/~raquel/Hawaiiposter.pdf
Jets and Outflows in Protoplanetary Disks Raquel Salmeron(1), Arieh KЖnigl(2) & Mark Wardle(3) (1) Research School of Astronomy & Astrophysics and Research School of Earth Sciences, ANU (2) Dept. ... They are thought to be launched centrifugally from the disk surfaces via the stresses of open magnetic field lines that thread the disk [3]. However, in protoplanetary disks the ionization fraction is low and the ability of the field to couple to the gas (and drive a wind) is severely limited. ...
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Ссылки http://www.mso.anu.edu.au/~raquel/Hawaiiposter.pdf -- 159.5 Кб -- 06.01.2008
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3225. http://www.mso.anu.edu.au/~bessell/FTP/Anna/in.lis
sp113bs sp114bs sp115bs sp116bs sp117bs sp118bs sp119bs sp120bs sp121bs sp145bs sp146_7bs sp148bs sp149bs
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Anna/in.lis -- 1.1 Кб -- 18.12.2007
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3226. http://www.mso.anu.edu.au/~jerjen/researchprojects/spinningsun/Tang.pdf
ROTATION RATE OF HIGH-LATITUDE FRANCES TANG SUNSPOTS Hale Observatories,* California Institute of Technology, Pasadena, Calif. ... Rotation rate of 19 high latitude (28~,4 ~ short-lived sunspots collected in 1978-1979 are compared with Newton and Nunn's (1951) recurrent spots rate. ... Introduction The solar rotation rate for spots derived from recurrent sunspots in the solar cycle 1934-44 by Newton and Nunn (1951) has long been a classic. ... 5) In the 40-45 ~ latitude zone we have only two spots. ...
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Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/spinningsun/Tang.pdf -- 277.3 Кб -- 05.12.2007
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3227. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l745-46a.tab
L745-46A l745.bbfits * set .z.units = Ergs/s/cm**2/A set .z.label = Flux set .table.bandwidth = 50 * 3050.000 3.504e+15 3100.000 3.529e+15 3150.000 3.553e+15 3200.000 3.569e+15 3250.000 3.580e +15 3300.000 3.589e+15 3350.000 3.594e+15 3400.000 3.593e+15 3450.000 3.587e+15 3500.000 3.580e +15 3550.000 3.571e+15 3600.000 3.556e+15 3650.000 3.540e+15 3700.000 3.519e+15 3750.000 3.499e+15 3800.000 3.474e+15 3850.000 3 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/l745-46a.tab -- 4.4 Кб -- 13.11.2007
[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l745-46a.tab -- 4.4 Кб -- 13.11.2007
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[ Сохраненная копия ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/l745-46a.tab -- 4.4 Кб -- 13.11.2007
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3228. http://www.mso.anu.edu.au/~charley/papers/ConvergenceIntelligence10.pdf
... Meanwhile, three species of apes (chimps, gorillas and orangutans) learn to speak English, rid e horses, farm corn, shoot rifles, and in gen eral begin to act like h airy Victor ian humano ids with human-like intellig ence. ... Is human-like intellig ence a convergent featur e of evolution? ... All together th at makes about 3 billion years of prokaryotic evo lution that did not produce high intelligence and about 600 million years of protist evolution th at did no t produce high intellig ence. ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/ConvergenceIntelligence10.pdf -- 371.5 Кб -- 12.11.2007
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3229. http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver2007.pdf
... Printed in U.S.A. THE METALLICITY OF STARS WITH CLOSE COMPANIONS Daniel Grether1 and Charles H. Lineweaver2 Received 2006 November 30; accepted 2007 July 5 ABSTRACT We examine the relationship between the frequency of close companions (stellar and planetary companions with orbital periods <5 yr) and the metallicity of their Sun-like ($FGK ) hosts. ... In contrast to the metallicity dependence of planetary companions, stellar companions tend to be more abundant around low-metallicity hosts. ... Fig. ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/GretherLineweaver2007.pdf -- 693.4 Кб -- 04.11.2007
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3230. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/bessell2007BJ.pdf
... Printed in U.S.A. Measuring the Balmer Jump and the Effective Gravity in FGK Stars Michael S. Bessell Research School of Astronomy and Astrophysics, Australian National University, Mount Stromlo, Weston, Australia; bessell@mso.anu.edu.au Received 2006 October 17; accepted 2007 May 18; published 2007 June 21 ABSTRACT. ... Synthetic fl spectra for [Fe/H] p 2.5, 5750 K, and log g p 4.5, 3.5, 2.5. ... Synthetic spectra divided by an 11,800 K BB for [Fe/H] p 2.5, 6500 K, and log g p 4.5, 4.0, 2.5. ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/bessell2007BJ.pdf -- 282.6 Кб -- 08.10.2007
[ Текст ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/bessell2007BJ.pdf -- 282.6 Кб -- 08.10.2007
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[ Текст ] Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/bessell2007BJ.pdf -- 282.6 Кб -- 08.10.2007
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3231. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/spectro.coord
... 15318 B9III 4.279 -0.056 -0.107 -0.023 -0.063 xi Cet "bs1544" 04 50 36.7 08 54 01 J2000.0 ! ... 34 239 sdG 11.225 0.488 -0.058 0.295 0.587 -0.030 -0.245 H "VMa2" 00 49 10 +05 23.4 J2000.0 ! 0046+051 LHS 7 DZ7 12.382 0.550 0.006 0.255 0.499 0.0812 -2.722 O "LTT1020" 01 54 48 -27 28.7 J2000.0 ! ... 2317-054 sdO 11.846 -0.304 -1.153 -0.133 -0.325 H,O !! ! ... 00 47 03.6487 -11 52 21.558 J2000.0(1999.5) 0.0 0.0 0.0 0.0 "BD-12" 00 52 15.3737 -10 39 48.039 J2000.0(1999.5) 0.0 0.0 0.0 0.0 "BD-11" ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/spectro.coord -- 11.3 Кб -- 08.10.2007
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3232. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/VMa2_modela.txt
... Ser. 27,21 # by adding a constant offset in m_AB. The offset is determined for the region # 5250-9200 Angstroms. ... SET .Z.UNITS = mjy SET .Z.LABEL = Fnu SET .TABLE.BANDWIDTH = 50 SET .TABLE.LAMBDA_DOUBLE = 11000 * 3050.000 2.741 3100.000 5.483 3150.000 7.639 3200.000 9.151 3250.000 10.653 3300.000 11.985 3350.000 13.154 3400.000 13.901 3450.000 13.142 3500.000 14.718 3550.000 14.992 3600.000 14.637 3650.000 15.756 3700.000 14.370 3750.000 9.787 3800 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/VMa2_modela.txt -- 4.2 Кб -- 08.10.2007
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3233. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/VMa2_model.txt
... Ser. 27, 21 # by adding a constant offset in m_AB. The offset is determined for the region # 5250-9200 Angstroms. Not recommended shordward of 4250 Angstroms. There are strong features in # the region 3750-4250 Angstroms , and there is an offset of Oke from the # model shortward of 3750 Angstroms , where m_AB varies very rapidly with # wavelength # SET .Z.UNITS = AB magnitudes SET .Z.LABEL = Flux SET .Z.REVSCALE = 1 SET .Z.MAGFLAG = 1 SET .TABLE.BANDWIDTH = 50 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/VMa2_model.txt -- 4.5 Кб -- 08.10.2007
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3234. http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/vma2a.tab
... 55 4690 12.52 4700 12.51 4710 12.50 4720 12.50 4730 12.50 4740 12.48 4750 12.48 4760 12.50 4770 12.48 4780 12.47 4790 12.45 4800 12.43 4810 12.43 4820 12.43 4830 12.43 4840 12.41 4850 12.45 4860 12.44 4870 12.44 4880 12.44 4890 12.42 4900 12.43 4910 12.43 4920 12.46 4930 12.44 4940 12.46 4950 12.42 4960 12.43 4970 12.44 4980 12.45 4990 12.45 5000 12.45 5010 12.44 5020 12.46 5030 12.47 5040 12.47 5050 12.47 5060 12.46 5070 12.45 5080 12 ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Oldspectrophotometry/vma2a.tab -- 6.2 Кб -- 08.10.2007
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3235. http://www.mso.anu.edu.au/~raquel/GRC_poster_5.pdf
... 1) The conductivity tensor Left panel: No grains are present. ... Right Panel: 0.1 m grains are present. ... Right panel: Growth rates of the fastest growing modes at 1 AU as a function of the strength of the magnetic field for different configurations of the conductivity tensor (b) Effect of dust grains (R = 5 AU) (1b) H H H H When dust grains are present, MRI modes grow for B < 80 mG (a=1 m) and B < 15 mG (0.1 m), down from B < 800 mG when grains are assumed to be settled (see section 3a, above). ...
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Ссылки http://www.mso.anu.edu.au/~raquel/GRC_poster_5.pdf -- 1425.4 Кб -- 13.09.2007
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3236. http://www.mso.anu.edu.au/~brian/A3002/lect15.pdf
... At any given time... s peed of sound * age of Universe creates a s o u n d - h o r iz o n , c o h e r e n t s c a le s w h e r e m a tte r is fa llin g in fo r th e fi r s t tim e , on smaller scales, matter has reverberated in and out.. ... Like a fourier series, the amplitude of the different scales, tells you the power (the strength) of the fluctuations on different scales. ... B e a m p a tte rn b y o b s e r v in g u n c e r ta in tie s p a tte rn a ffe c t fu n c tio n . ...
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Ссылки http://www.mso.anu.edu.au/~brian/A3002/lect15.pdf -- 2186.3 Кб -- 28.08.2007
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3237. http://www.mso.anu.edu.au/~brian/A3002/probset2.pdf
... Problem 1.1: (4pts) We want to use supernovae as a standard candle to measure luminosity distance as a function of redshift in order to determine the Hubble Constant. ... Problem 2: In a flat Universe, the luminosity distance to an object at redshift z, in a universe made up of i forms of matter each with an equation of state wi and density, i is given by ,1 / 2 z & ) c 3 + 3wi DL = (1 + z) # dz"(% $i (1 + z") + H0 'i * 0 2.1 (5 pts). ... Assume the universe is radiation dominated the whole time. ...
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Ссылки http://www.mso.anu.edu.au/~brian/A3002/probset2.pdf -- 181.9 Кб -- 26.08.2007
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3238. http://www.mso.anu.edu.au/~bessell/FTP/Hipparcos/bessell_hip_PASP.pdf
... Printed in U.S.A. The Hipparcos and Tycho Photometric System Passbands MICHAEL S. BESSELL Research School of Astronomy and Astrophysics, Institute of Advanced Studies, The Australian National University, Private Bag, Weston Creek P.O., ACT 2611, Australia ; bessell=mso.anu.edu.au Received 2000 March 6 ; accepted 2000 April 17 ABSTRACT. Hipparcos and T ycho magnitudes have been extracted for many of the E-region standard stars. ... B [V regression for the E-region stars. ...
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Ссылки http://www.mso.anu.edu.au/~bessell/FTP/Hipparcos/bessell_hip_PASP.pdf -- 269.2 Кб -- 22.08.2007
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3239. http://www.mso.anu.edu.au/~kcf/surya/Sellwood.Deb06.pdf
Revised version submitted to ApJ A Preprint typ eset using L TEX style emulateap j v. 04/03/99 BAR - HALO FRICTION IN GALAXIES II: METASTABILITY J. A. Sellwood Rutgers University, Department of Physics Astronomy, 136 Frelinghuysen Road, ... .washington.edu arXiv:astro-ph/0511155v1 5 Nov 2005 Revised version submitted to ApJ ABSTRACT It is well-established that strong bars rotating in dense halos generally slow down as they lose angular momentum to the ... Fig. ... As the sim- 10 Fig. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/surya/Sellwood.Deb06.pdf -- 432.4 Кб -- 31.07.2007
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3240. http://www.mso.anu.edu.au/~kcf/surya/swaters00
... Mass modeling shows that the contribution of the stellar component to the rotation cur ves may be scaled to explain most of the inner parts of the rotation cur ves, albeit with high stellar mass-to-light ratios. ... L107 L108 HIGH-RESOLUTION ROTATION CURVES Vol. ... The relative contribution of the stellar disk to the rotation cur ve may change continuously from LSB to HSB, or perhaps LSB and HSB galaxies constitute discrete galaxy families, as has been suggested by Tully & Verheijen (1997). ...
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Ссылки http://www.mso.anu.edu.au/~kcf/surya/swaters00 -- 112.4 Кб -- 31.07.2007
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