Galaxy rotation curve

Results: 59



#Item
1dark matter in spiral galaxies mass, size and shape of the halo rotation curves • extended (core/cusp: Nancy)

dark matter in spiral galaxies mass, size and shape of the halo rotation curves • extended (core/cusp: Nancy)

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Source URL: www.astro.rug.nl

Language: English - Date: 2011-05-16 03:37:41
2Vrije Universiteit Brussel Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde Study of the sensitivity

Vrije Universiteit Brussel Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde Study of the sensitivity

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Source URL: web.iihe.ac.be

Language: English - Date: 2013-11-25 11:10:48
3Morphology and Dynamics of Galaxies with Cellular Automata Dr.  Brian  R.  Kent  (Na#onal  Radio  Astronomy  Observatory)   Abstract Galaxies are among the largest observed physical systems, surpa

Morphology and Dynamics of Galaxies with Cellular Automata Dr.  Brian  R.  Kent  (Na#onal  Radio  Astronomy  Observatory)   Abstract Galaxies are among the largest observed physical systems, surpa

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Source URL: www.wolframscience.com

Language: English - Date: 2011-12-20 16:47:23
4CHANGING IT IS TIME FOR WDM Paolo Salucci SISSA DARK MATTER IN GALAXIES

CHANGING IT IS TIME FOR WDM Paolo Salucci SISSA DARK MATTER IN GALAXIES

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Source URL: chalonge.obspm.fr

Language: English - Date: 2014-06-10 09:25:26
5Galaxy Structure Observations and Cored Density Profiles CHANGING IT IS TIME FOR WDM

Galaxy Structure Observations and Cored Density Profiles CHANGING IT IS TIME FOR WDM

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Source URL: chalonge.obspm.fr

Language: English - Date: 2014-07-28 03:26:13
6LWDM. Warm Dark Matter Galaxy Theory inAgreement with Observations. Norma G. SANCHEZ DR CNRS LERMA Observatoire de Paris

LWDM. Warm Dark Matter Galaxy Theory inAgreement with Observations. Norma G. SANCHEZ DR CNRS LERMA Observatoire de Paris

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Source URL: chalonge.obspm.fr

Language: English - Date: 2014-07-28 03:26:14
7Ay 124 – Handouts 3 Asymmetric Drift and Star Streams Dehnen & Binney found that the V component (in the plane) of the sun’s motion depends on what kind of local

Ay 124 – Handouts 3 Asymmetric Drift and Star Streams Dehnen & Binney found that the V component (in the plane) of the sun’s motion depends on what kind of local

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Source URL: www.tapir.caltech.edu

Language: English - Date: 2010-01-31 22:52:23
8Vrije Universiteit Brussel Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde Study of the sensitivity

Vrije Universiteit Brussel Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde Study of the sensitivity

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Source URL: www.iihe.ac.be

Language: English - Date: 2013-11-25 11:10:48
9Vrije Universiteit Brussel Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde Study of the sensitivity

Vrije Universiteit Brussel Faculteit Wetenschappen en Bio-ingenieurswetenschappen Departement Natuurkunde Study of the sensitivity

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Source URL: iihe.ac.be

Language: English - Date: 2013-11-25 11:10:48
10Qualification Examination—Galactic and Extragalactic Astronomy May, Motion of the Galaxy: (a) How do we know the sun is moving with respect to the nearby stars, i.e., how do we know the motion of the sun relati

Qualification Examination—Galactic and Extragalactic Astronomy May, Motion of the Galaxy: (a) How do we know the sun is moving with respect to the nearby stars, i.e., how do we know the motion of the sun relati

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Source URL: www.astro.ncu.edu.tw

Language: English - Date: 2014-05-12 00:06:46