✦ LIBER ✦

The fundamental plane of elliptical galaxies with modified Newtonian dynamics

✍ Scribed by R. H. Sanders

Publisher: John Wiley and Sons
Year: 2000
Tongue: English
Weight: 328 KB
Volume: 313
Category: Article
ISSN: 0035-8711
DOI: 10.1046/j.1365-8711.2000.03272.x

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The near-infrared Fundamental Plane of e

The near-infrared Fundamental Plane of elliptical galaxies

✍ B. Mobasher; R. Guzmán; A. Aragón-Salamanca; S. Zepf 📂 Article 📅 1999 🏛 John Wiley and Sons 🌐 English ⚖ 830 KB

Clusters of galaxies with modified Newto

Clusters of galaxies with modified Newtonian dynamics

✍ R. H. Sanders 📂 Article 📅 2003 🏛 John Wiley and Sons 🌐 English ⚖ 178 KB

Radial orbital anisotropy and the Fundam

Radial orbital anisotropy and the Fundamental Plane of elliptical galaxies

✍ C. Nipoti; P. Londrillo; L. Ciotti 📂 Article 📅 2002 🏛 John Wiley and Sons 🌐 English ⚖ 260 KB

Mergers between elliptical galaxies and

Mergers between elliptical galaxies and the thickening of the Fundamental Plane

✍ A. C. González-García; T. S. Van Albada 📂 Article 📅 2003 🏛 John Wiley and Sons 🌐 English ⚖ 493 KB

Galaxy merging, the fundamental plane of

Galaxy merging, the fundamental plane of elliptical galaxies and the MBH−σ0 relation

✍ C. Nipoti; P. Londrillo; L. Ciotti 📂 Article 📅 2003 🏛 John Wiley and Sons 🌐 English ⚖ 330 KB

Dark matter and modified Newtonian dynam

Dark matter and modified Newtonian dynamics in a sample of high-redshift galaxy clusters observed with Chandra

✍ Carl Blaksley; Massimiliano Bonamente 📂 Article 📅 2010 🏛 Elsevier Science 🌐 English ⚖ 927 KB

We compare the measurement of the gravitational mass of 38 high-redshift galaxy clusters observed by Chandra using Modified Newtonian Dynamics (MOND) and standard Newtonian gravity. Our analysis confirms earlier findings that MOND cannot explain the difference between the baryonic mass and the total