Stellar structure

Results: 127



#Item
81Matter / Exotic matter / Active galactic nucleus / Stellar evolution / Galaxy / Structure formation / White dwarf / Redshift / Physics / Physical cosmology / Astronomy

The growth of galaxies and their gaseous haloes Freeke van de Voort The growth of galaxies and

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Source URL: home.strw.leidenuniv.nl

Language: English - Date: 2012-03-13 09:23:59
82Physical cosmology / Large-scale structure of the cosmos / Exotic matter / Galaxies / Dark matter / Active galactic nucleus / Galaxy groups and clusters / Quasar / Accretion / Physics / Astronomy / Stellar evolution

2 The rates and modes of gas accretion onto galaxies and their gaseous haloes We study the rate at which gas accretes onto galaxies and haloes and investigate whether the accreted gas was shocked to high temperatures bef

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Source URL: home.strw.leidenuniv.nl

Language: English - Date: 2012-03-13 09:13:49
83Dark matter / Exotic matter / Stellar evolution / Astrophysics / Galaxy groups and clusters / Galaxy formation and evolution / Galaxy / Active galactic nucleus / Physical cosmology / Physics / Astronomy / Large-scale structure of the cosmos

4 Properties of gas in and around galaxy haloes We study the properties of gas inside and around galaxy haloes as a function of radius and halo mass, focusing mostly on z = 2, but also showing some results for z = 0. For

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Source URL: home.strw.leidenuniv.nl

Language: English - Date: 2012-03-13 09:15:02
84Large-scale structure of the cosmos / Stellar evolution / Exotic matter / Dark matter / Active galactic nucleus / Galaxy groups and clusters / Quasar / Accretion / Black hole / Physics / Astronomy / Galaxies

3 The drop in the cosmic star formation rate below redshift 2 is caused by a change in the mode of gas accretion and by active galactic nucleus feedback

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Source URL: home.strw.leidenuniv.nl

Language: English - Date: 2012-03-13 09:14:25
85Large-scale structure of the cosmos / Galaxies / Stellar evolution / Radio astronomy / Dark matter / Active galactic nucleus / Galaxy groups and clusters / Galaxy formation and evolution / Quasar / Physics / Astronomy / Physical cosmology

1 Introduction Galaxy formation has undergone fast development in the past few decades, both theoretically and observationally. The number of observed galaxies is expanding rapidly and observations are pushing to lower m

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Source URL: home.strw.leidenuniv.nl

Language: English - Date: 2012-03-13 09:12:07
86Space / Light sources / Astrophysics / Sun / Helioseismology / Stellar structure / Star / Stellar evolution / Angular momentum / Stellar astronomy / Physics / Astronomy

Astronomy & Astrophysics A&A 554, A40[removed]DOI: [removed][removed]

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Source URL: www.aanda.org

Language: English
87

Stellar Structure and Evolution Examples 5 : due Monday April 7 1. Derive an expression for the exponential factor in the penetration probability (this equals (−2πη) in KW eqn[removed]in terms of the classical turn-aro

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Source URL: www.pha.jhu.edu

- Date: 2014-03-29 12:54:26
    88Sun / Plasma physics / Space plasmas / Helioseismology / Astrophysics / Space telescopes / Asteroseismology / COROT / Stellar structure / Astronomy / Space / Physics

    NSO Workshop # 27: Fifty Years of Seismology of the Sun and Stars May 6 – 10, 2013, Westin La Paloma, Tucson, AZ, USA Scientific Program Day 1: May 6, 2013, Monday 16:[removed]:30

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    Source URL: www.nso.edu

    Language: English - Date: 2013-05-16 20:18:11
    89Physical cosmology / Large-scale structure of the cosmos / Galaxy formation and evolution / Stellar evolution / MRC 1138-262 / Galaxy / Radio galaxy / Cosmic distance ladder / Spiral galaxy / Astronomy / Extragalactic astronomy / Space

    The Astrophysical Journal, 650: L29–L32, 2006 October 10 䉷 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE SPIDERWEB GALAXY: A FORMING MASSIVE CLUSTER GALAXY AT z ∼ 2 George K. M

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    Source URL: www.spacetelescope.org

    Language: English - Date: 2006-10-10 09:40:10
    90

    Stellar Structure and Evolution Examples 2 : due Friday Feb 28, 5pm 1. (a) Calculate the ratio of (ideal) gas pressure to radiation pressure in the interior of the Sun, taking suitable ‘interior’ values for the param

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    Source URL: www.pha.jhu.edu

    - Date: 2014-02-21 20:08:57
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