1![dark 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)](https://www.pdfsearch.io/img/55bcdc562827ad6213c2a96368519baf.jpg) | Add to Reading ListSource URL: www.astro.rug.nlLanguage: English - Date: 2011-05-16 03:37:41
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2![Vrije 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](https://www.pdfsearch.io/img/e3239bebcb5a46943b41dd70d5800033.jpg) | Add to Reading ListSource URL: web.iihe.ac.beLanguage: English - Date: 2013-11-25 11:10:48
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3![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 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](https://www.pdfsearch.io/img/8be0c9e39340bb431c071876395d9111.jpg) | Add to Reading ListSource URL: www.wolframscience.comLanguage: English - Date: 2011-12-20 16:47:23
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4![CHANGING 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](https://www.pdfsearch.io/img/bec1016b3709afca92ef386adc343c19.jpg) | Add to Reading ListSource URL: chalonge.obspm.frLanguage: English - Date: 2014-06-10 09:25:26
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5![Galaxy 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](https://www.pdfsearch.io/img/336ceb6515a1a488fb609d5dd45b053a.jpg) | Add to Reading ListSource URL: chalonge.obspm.frLanguage: English - Date: 2014-07-28 03:26:13
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6![LWDM. 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](https://www.pdfsearch.io/img/2206528b05b23c8f31a004be2a16c3a9.jpg) | Add to Reading ListSource URL: chalonge.obspm.frLanguage: English - Date: 2014-07-28 03:26:14
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7![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 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](https://www.pdfsearch.io/img/20d030345168ca60488657ca9f8e605e.jpg) | Add to Reading ListSource URL: www.tapir.caltech.eduLanguage: English - Date: 2010-01-31 22:52:23
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8![Vrije 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](https://www.pdfsearch.io/img/da0a9cb8cabbabf5f3eaf2435d2ff473.jpg) | Add to Reading ListSource URL: www.iihe.ac.beLanguage: English - Date: 2013-11-25 11:10:48
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9![Vrije 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](https://www.pdfsearch.io/img/87d25090c8d0813b6b4267a9b23715fb.jpg) | Add to Reading ListSource URL: iihe.ac.beLanguage: English - Date: 2013-11-25 11:10:48
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10![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 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](https://www.pdfsearch.io/img/60981c9fd1f43c8edaa757bacfaef887.jpg) | Add to Reading ListSource URL: www.astro.ncu.edu.twLanguage: English - Date: 2014-05-12 00:06:46
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