Stellar density

Results: 31



#Item
21Verification of SCIAMACHY lv1b V6 nadir data

Verification of SCIAMACHY lv1b V6 nadir data

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Source URL: www.iup.uni-bremen.de

Language: English - Date: 2007-01-22 09:25:56
22Smoothed Particle Hydrodynamics and Magnetohydrodynamics Daniel J. Price Centre for Stellar and Planetary Astrophysics & School of Mathematical Sciences, Monash University, Melbourne Vic. 3800, Australia  Abstract

Smoothed Particle Hydrodynamics and Magnetohydrodynamics Daniel J. Price Centre for Stellar and Planetary Astrophysics & School of Mathematical Sciences, Monash University, Melbourne Vic. 3800, Australia Abstract

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Source URL: users.monash.edu.au

Language: English - Date: 2010-12-08 17:21:11
23Homework #1 1. The density of the interior of the sun is significantly larger than that of water. a) Provide a quantitative relation between the temperature and density of a star which indicates when we can treat it as a

Homework #1 1. The density of the interior of the sun is significantly larger than that of water. a) Provide a quantitative relation between the temperature and density of a star which indicates when we can treat it as a

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Source URL: astro.berkeley.edu

Language: English - Date: 2013-01-28 21:05:13
245 Cold accretion flows and the nature of high column density H i absorption at redshift 3 Simulations predict that galaxies grow primarily through the accretion of gas that has not gone through an accretion shock near th

5 Cold accretion flows and the nature of high column density H i absorption at redshift 3 Simulations predict that galaxies grow primarily through the accretion of gas that has not gone through an accretion shock near th

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Source URL: home.strw.leidenuniv.nl

Language: English - Date: 2012-03-13 09:15:30
257  A Mathematical Model of the Sun Once an astronomer knows the radius and mass of a planet or star, one of

7 A Mathematical Model of the Sun Once an astronomer knows the radius and mass of a planet or star, one of

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Source URL: spacemath.gsfc.nasa.gov

Language: English - Date: 2009-02-20 13:17:34
26Color Plate 1. Sample density, velocity, and magnetic field structure in two turbulent cloud simulations. Density contours are logarithmic, with dark blue running from the mean density to ten times the mean, and light bl

Color Plate 1. Sample density, velocity, and magnetic field structure in two turbulent cloud simulations. Density contours are logarithmic, with dark blue running from the mean density to ten times the mean, and light bl

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Source URL: www.uapress.arizona.edu

Language: English - Date: 2007-04-05 13:30:42
27Full Papers  Experientia[removed]), Birkh/iuser Verlag, CH-4010 Basel/Switzerland I Butenandt, A., Jb. preuss. Akad. Wiss[removed]Butenandt, A., Naturw. Rdsch. Stuttg[removed].

Full Papers Experientia[removed]), Birkh/iuser Verlag, CH-4010 Basel/Switzerland I Butenandt, A., Jb. preuss. Akad. Wiss[removed]Butenandt, A., Naturw. Rdsch. Stuttg[removed].

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Source URL: rdbiotech.drivehq.com

Language: English - Date: 2007-08-19 19:43:59
28Equation of State Calculations of Hydrogen-Helium Mixtures in Solar and Extrasolar Giant Planets Burkhard Militzer1 1 Department of Earth and Planetary Science, Department of Astronomy, University of California, Berkeley

Equation of State Calculations of Hydrogen-Helium Mixtures in Solar and Extrasolar Giant Planets Burkhard Militzer1 1 Department of Earth and Planetary Science, Department of Astronomy, University of California, Berkeley

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Source URL: militzer.berkeley.edu

Language: English - Date: 2013-01-10 12:04:43
29Webfooted Astronomer News from the Seattle Astronomical Society August 2007 Density is destiny The UW’s Dr. Eric Agol tells SAS all about

Webfooted Astronomer News from the Seattle Astronomical Society August 2007 Density is destiny The UW’s Dr. Eric Agol tells SAS all about

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Source URL: archive.seattleastro.org

Language: English - Date: 2013-05-24 12:10:51
30Energy rate density as a complexity metric and evolutionary driver

Energy rate density as a complexity metric and evolutionary driver

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Source URL: www.cfa.harvard.edu

Language: English - Date: 2011-06-14 12:15:57