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3081. http://www.mso.anu.edu.au/~kcf/pubs_top20/95.pdf
... We explore here models based upon helium stars in the range 9х14 M and carbon-oxygen stars 6х11 M , _ _ which experience unusually energetic explosions (kinetic energy 0.5 х2.8 ] 1052 ergs). ... However, the high explosion energies required to understand the supernova are in contrast to what is expected for such massive stars and indicate that a new sort of explosion may have been identiпed, possibly the consequence of a collapsar. ... In toto, the case for a GRB-supernova association is compelling....
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/95.pdf -- 160.2 Кб -- 16.10.2011
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3082. http://www.mso.anu.edu.au/~kcf/pubs_top20/94.pdf
... Printed in U.S.A. OPTICAL AND RADIO OBSERVATIONS OF THE AFTERGLOW FROM GRB 990510: EVIDENCE FOR A JET F. A. Harrison,1 J. S. Bloom,1 D. A. Frail,2 R. Sari,3 S. R. Kulkarni,1 S. G. Djorgovski,1 T. Axelrod ... . McConnell,5 P. J. McCarthy,6 B. E. Schaefer,7 R. G. McMahon,8 R. O. Markze,6 E. Firth,8 P. Soffitta,9 and L. Amati10 Received 1999 July 12; accepted 1999 August 2; published 1999 September 7 ABSTRACT We present multicolor optical and two-frequency ... 1999; Amati et al. ... 1999)...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/94.pdf -- 76.2 Кб -- 16.10.2011
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3083. http://www.mso.anu.edu.au/~kcf/pubs_top20/91.pdf
... The set of D30 new, unпltered CCD observations delineate the early rise behavior of SNe Ia 18 to 10 days before maximum. ... Using a variety of light-curve shape methods, we пnd the rise time to B maximum for an SN Ia with *m (B) \ 1.1 mag and peak M \[19.45 mag to be 19.5 ^ 0.2 days. ... OBSERVATIONS 2.1. ... 118 V B mag 20 -20 -10 0 10 Age (Days) 20 FIG. 4.хL eft : Observed V -band light curves for 10 SNe Ia including rise-time observations transformed from unпltered CCD measurements. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/91.pdf -- 432.7 Кб -- 16.10.2011
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3084. http://www.mso.anu.edu.au/~kcf/pubs_top20/27.pdf
... Printed in U.S.A. HUBBLE SPACE TELESCOPE AND SPITZER OBSERVATIONS OF THE AFTERGLOW AND HOST GALAXY OF GRB 050904 AT z = 6.295 E. Berger, 1,2,3 R. Chary,4 L. L. Cowie,5 P. A. Price,5 B. P. Schmidt,6 D. B. Fox,7 S. B. Cenko, S. G. Djorgovski,9 ... 2005). ... 11 102 AFTERGLOW AND HOST GALAXY OF GRB 050904 103 Fig. ... 1, 2007 AFTERGLOW AND HOST GALAXY OF GRB 050904 105 Fig. ... We find that in the published sample, only 14 galaxies are located at a higher redshift than the host of GRB 050904....
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/27.pdf -- 711.2 Кб -- 16.10.2011
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3085. http://www.mso.anu.edu.au/~kcf/pubs_top20/87.pdf
... Printed in U.S.A. TESTS OF THE ACCELERATING UNIVERSE WITH NEAR-INFRARED OBSERVATIONS OF A HIGH-REDSHIFT TYPE Ia SUPERNOVA ADAM G. RIESS ,1 ALEXEI V. FILIPPENKO,2 MICHAEL C. LIU,2 PETER CHALLIS,3 ALEJANDRO CLOCCHIATTI,4 ALAN DIERCKS,5 PETER M. GARNAVICH,3 CRAIG J. HOGAN ... 1998 ; Perlmutter et al. ... The telltale signature of extinction by Galactic-type dust, reddening, has not been detected in the amount required to provide A \ 0.3 mag for high-z SNe Ia (Riess et al. ... 1998, 1999 ; Riess et...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/87.pdf -- 91.9 Кб -- 16.10.2011
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3086. http://www.mso.anu.edu.au/~kcf/pubs_top20/80.pdf
THE ASTROPHYSICAL JOURNAL, 560 : 49 х 71, 2001 October 10 ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A. V THE FARTHEST KNOWN SUPERNOVA : SUPPORT FOR AN ACCELERATING UNIVERSE AND A GLIMPSE OF THE EPOCH OF DECELERATION1 ADAM G. RIESS,2 PETER E. NUGENT,3 RONALD L. GILLILAND,2 BRIAN P. SCHMIDT,4 JOHN TONRY,5 MARK DICKINSON,2 RODGER I. THOMPSON,6 TAMAS BUDAVARI,7 STEFANO CASERTANO,2 AARON S. EVANS,8 ALEXEI V. FILIPPENKO,9 MARIO LIVIO,2 DAVID B. SANDERS,5 ALICE E. SHAPLEY,10
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/80.pdf -- 1679.9 Кб -- 16.10.2011
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3087. http://www.mso.anu.edu.au/~kcf/pubs_top20/67.pdf
The Astrophysical Journal, 594: 1-24, 2003 September 1 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. E COSMOLOGICAL RESULTS FROM HIGH-z SUPERNOVAE 1,2 7 John L. Tonry,3 Brian P. Schmidt,4 Brian Barris,3 Pablo Candia,5 Peter Challis,6 Alejandro Clocchiatti, Alison L. Coil,8 Alexei V. Filippenko,8 Peter Garnavich,9 Craig Hogan,10 Stephen T. Holland,9 Saurabh Jha,6,8 Robert P. Kirshner,6 Kevin Krisciunas,5,11 Bruno Leibundgut,12 Weidong Li,8 Thomas Matheson,6 Mark M.
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/67.pdf -- 1043.4 Кб -- 16.10.2011
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3088. http://www.mso.anu.edu.au/~kcf/pubs_top20/53.pdf
Publications of Brian P. Schmidt: top 20 * 2. ... Tonry, John L., Schmidt , Brian P., Barris, Brian , Candia, Pablo, Challis, Peter , Cloc c hiatti, Alejandro, Coil, Alison L., Filippenko , Alexei V., Garnavich, Peter , Hogan, Craig, Holland, Stephen T., Jha, Saurabh, Kirshner , Robert P., Kris ciunas, Kevin, Leibundgut, Bruno, Li, Weidong, Matheson, Thomas, Phillips , Mark M., Ries s , Adam G., Schommer, ...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/53.pdf -- 65.4 Кб -- 16.10.2011
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3089. http://www.mso.anu.edu.au/~kcf/pubs_top20/69.pdf
Discovery of the Bright Afterglow of the Nearby Gamma-Ray Burst of 29 March 2003 P. A. Price1, D. W. Fox2, S. R. Kulkarni2, B. A. Peterson1, B. P. Schmidt1, A. M. Soderberg2, S. A. Yost3, E. Berger2, S. G. Djorgovski2, D. A. Frail4, F. A. Harrison3, R. Sari5, A. W. Blain2, and S. C. Chapman2. 1 2 3 4 5 arXiv:astro-ph/0309419v1 16 Sep 2003 RSAA, ANU, Mt. ... Figure 1: Discovery of the bright optical afterglow of GRB 030329. ... Figure 4: Light-curve of the optical afterglow of GRB 030329. ... Figure 1. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/69.pdf -- 471.3 Кб -- 15.10.2011
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3090. http://www.mso.anu.edu.au/~kcf/pubs_top20/54.pdf
The afterglow of GRB 050709 and the nature of the short-hard -ray bursts D. B. Fox1 ,2 D. A. Frail,3 P. A. Price,4 S. R. Kulkarni,1 E. Berger,5 T. Piran,1 ,6 A. M. Soderb erg,1 S. B. Cenko,1 P. B. Cameron ... California, Berkeley, CA 94720, USA 10 11 12 13 14 15 16 17 18 19 The final chapter in the long-standing mystery of the gamma-ray bursts (GRBs) centres on the origin of the short-hard class, susp ected on theoretical grounds to result from the coalescence of neutron ...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/54.pdf -- 330.7 Кб -- 15.10.2011
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3091. http://www.mso.anu.edu.au/~kcf/pubs_top20/2.pdf
A PHOTOMETRIC REDSHIFT OF z 9.4 FOR GRB 090429B A. Cucchiara1,2,3 , A. J. Levan4 , D. B. Fox1 , N. R. Tanvir5 , T. N. Ukwatta6,7 , E. Berger8 , T. Kruhler9,10 , A. Kup cu Yoldaе11 ... In this pap er we discuss the discovery and multi-wavelength follow-up of GRB 090429B. The afterglow was not visible in deep early optical imaging, but was found in deep IR observations starting 2.5 hr after the burst. ... 2010, 2011). ... A log of the H S T optical and NIR observations of the GRB 090429B field. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/2.pdf -- 744.0 Кб -- 15.10.2011
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3092. http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf
CSIRO PUBLISHING www.publish.csiro.au/journals/pasa Publications of the Astronomical Society of Australia, 2007, 24, 1ґ12 The SkyMapper Telescope and The Southern Sky Survey S. C. KellerA,B , B. P. SchmidtA , M. S. BessellA , P. G. ConroyA , P. FrancisA , A. GranlundA , E. KowaldA , A. P. OatesA , T ... On site there is a scheduling and data quality assurance system. ... Figure 1 shows a plan of the observatory site. ... The The SkyMapper Telescope and The Southern Sky Survey 3 2000 Table 1. ...
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Ссылки http://www.mso.anu.edu.au/~kcf/pubs_top20/34.pdf -- 664.4 Кб -- 15.10.2011
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3093. http://www.mso.anu.edu.au/~geoff/HEA/Fluid_Dynamics.pdf
... Fluid dynamics provides us with the capability of understanding the transport of mass, momentum and energy. ... 2 The fundamental fluid dynamics equations The equations of fluid dynamics are best expressed via conservation laws for the conservation of mass, momentum and energy. Fluid Dynamics 1/22 2.1 Conservation of mass n v S i Consider the rate of change of mass within a fixed volume. ... 3.1 The momentum flux in a viscous fluid The starting point for considering viscosity is the momentum flux. ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Fluid_Dynamics.pdf -- 49.9 Кб -- 29.09.2011
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3094. http://www.mso.anu.edu.au/~geoff/HEA/10_Accretion_Disks_I.pdf
... High Energy Astrophysics, Vol. ... In unaveraged from this is: ds kT ---- = ij v i j ґ q i i dt Using the relations: kTds = d ґ hd kTds = dh ґ dp High Energy Astrophysics : Accretion Disks I (6.1-1) (6.1-2) 51/60 implies: s + P kT = ґ ---------------= ґh t t t t t s h p = vi ґ vi kTv i xi xi xi ds p kT ---- = + hv i ґ v i dt t xi xi This energy equation then becomes: p + hv i ґ v i = ij v i j ґ q i i t xi xi High Energy Astrophysics : Accretion ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/10_Accretion_Disks_I.pdf -- 300.9 Кб -- 29.09.2011
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3095. http://www.mso.anu.edu.au/~geoff/HEA/Questions%201-8.pdf
High Energy Astrophysics Solutions to Exercises 1. ... P R c r The flux density received at point P is: F= I cos d c = I cos sin d d = I sin 2 =2 I 0 cos sin d c = R2 I ----r2 That is, we recover the inverse square law. ... F d = size of circular aperture I L Circular aperture L sec d d cos Projected aperture d cos d First calculate the solid angle of rays hitting P the back of the camera. ... Because of the delta-function, F =A Hence, for an unresolved source, the flux per beam F source. ...
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Ссылки http://www.mso.anu.edu.au/~geoff/HEA/Questions%201-8.pdf -- 138.6 Кб -- 09.09.2011
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3096. http://www.mso.anu.edu.au/~ralph/data/cool/ABOUT.txt
... FILE LIST 1) Collisonal Ionisation Equilibrium cooling functions as a function of metallicity are given in the files: mzero.cie : cie cooling for primordial hydrogen/helium mix log (T) = 4-8.5 m-00.cie : cie cooling for solar abundances mix log (T) = 4-8.5 m-05.cie : [Fe/H] = -0.5, solar /primordial average ratios m-10.cie : [Fe/H] = -1.0, primordial ratios (ie enhanced oxygen) m-15.cie : [Fe/H] = -1.5, primordial ...
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Ссылки http://www.mso.anu.edu.au/~ralph/data/cool/ABOUT.txt -- 5.5 Кб -- 08.08.2011
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3097. http://www.mso.anu.edu.au/~gdc/talks/LocalGroupWinterSchols.pdf
Our Local Group of Galaxies Gary Da Costa Research School of Astronomy & Astrophysics Mt Stromlo Observatory The Australian National University 1 The Local Group is our local Universe: It is a physical (i.e. gravitationally bound) association of at least ~50 galaxies (continues to increase as new satellites of the Milky Way and M31 are discovered) with a radius of ~1.3 Mpc. ... 8 4 How complete is the Local Group census? ... Dwarf Galaxies 18 9 How complete is the list of Milky Way dSph companions? ...
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Ссылки http://www.mso.anu.edu.au/~gdc/talks/LocalGroupWinterSchols.pdf -- 2231.9 Кб -- 28.06.2011
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3098. http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/questacon_2011.pdf
... Here comes the SKA. ... HI Gas and Star Formation neutral atomic hydrogen gas cloud (HI) molecular gas cloud (H2) star formation Redshift, Observing the Past The Expanding Universe Hubble`s Law redshift velocity related to distance ... (due to light travel time) Hubble`s Law redshift velocity related to distance distance related to age (due to light travel time) Atmospheric Transmission optical gamma rays, X-rays ultravio let infrared radio ...
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Ссылки http://www.mso.anu.edu.au/~plah/Home_Page_Stuff/files/questacon_2011.pdf -- 2383.4 Кб -- 19.05.2011
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3099. http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L20/Lecture20.pdf
The Three Commandments of Uncertainty Advanced Uncertainties 2 Clicker Channel 1 Friday, 8 April 2011 Applications of what we learned last time Ї Three laws.. Friday, 8 April 2011 1: Thou Shalt Use the Standard Deviation! ... Friday, 8 April 2011 So you see that a lot of the time you are outside a standard deviation Ї If the curve really is a Gaussian, then (on average) 68% of measurements should fall within one standard deviation, 95% within two and 99.7% within three. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L20/Lecture20.pdf -- 646.5 Кб -- 08.04.2011
[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/phys1101/Lectures/L20/Lecture20.pdf -- 646.5 Кб -- 08.04.2011
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[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/phys1101/Lectures/L20/Lecture20.pdf -- 646.5 Кб -- 08.04.2011
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3100. http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L19/Lecture19.pdf
Probability Distribution Functions Advanced Uncertainties, Part 1 Tuesday, 5 April 2011 Probability Distribution Functions Ї Ї Ї A way to be precise about what we don't know! ... Tuesday, 5 April 2011 What do we already know? ... Mean = 15 Range = 0 Number of students! ... Tuesday, 5 April 2011 A Gaussian Distribution Tuesday, 5 April 2011 Equation 1 -1( f (x) = e 2 2 x-? ) 2 Ї where f(x) is the probability distribution function for x. is the mean value of x, and is the standard deviation. ...
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Ссылки http://www.mso.anu.edu.au/pfrancis/phys1101/Lectures/L19/Lecture19.pdf -- 724.9 Кб -- 05.04.2011
[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/phys1101/Lectures/L19/Lecture19.pdf -- 724.9 Кб -- 05.04.2011
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[ Текст ] Ссылки http://www.mso.anu.edu.au/~pfrancis/phys1101/Lectures/L19/Lecture19.pdf -- 724.9 Кб -- 05.04.2011
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