Editing Galaxy rotation curve (section)

== Dark matter ==
{{main| Dark matter}}
While the observed galaxy rotation curves were one of the first indications that some mass in the universe may not be visible, many different lines of evidence now support the concept of cold dark matter as the dominant form of matter in the universe. Among the lines of evidence are [[mass-to-light ratio]]s which are much too low without a dark matter component, the amount of hot gas detected in galactic clusters by [[x-ray astronomy]], measurements of cluster mass with the [[Sunyaev–Zeldovich effect]] and with [[gravitational lensing]].<ref name=Peacock-1998>{{Cite book |last=Peacock |first=J. A. |url=https://www.cambridge.org/core/product/identifier/9780511804533/type/book |title=Cosmological Physics |date=1998-12-28 |publisher=Cambridge University Press |isbn=978-0-521-41072-4 |edition=1 |doi=10.1017/cbo9780511804533}}</ref>{{rp|368}} Models of the formation of galaxies are based on their dark matter halos.<ref name="Wechsler-2018">{{Cite journal |last1=Wechsler |first1=Risa H. |last2=Tinker |first2=Jeremy L. |date=2018-09-14 |title=The Connection Between Galaxies and Their Dark Matter Halos |url=https://www.annualreviews.org/doi/10.1146/annurev-astro-081817-051756 |journal=Annual Review of Astronomy and Astrophysics |language=en |volume=56 |issue=1 |pages=435–487 |doi=10.1146/annurev-astro-081817-051756 |arxiv=1804.03097 |issn=0066-4146 |quote=In our modern understanding of galaxy formation, every galaxy forms within a dark matter halo. }}</ref> The existence of [[cold dark matter|non-baryonic cold dark matter]] (CDM) is today a major feature of the [[Lambda-CDM model]] that describes the [[physical cosmology|cosmology]] of the [[universe]] and matches high precision astrophysical observations.<ref name=PDG-2024>{{Cite journal |last1=Navas |first1=S. |last2=Amsler |first2=C. |last3=Gutsche |first3=T. |last4=Hanhart |first4=C. |last5=Hernández-Rey |first5=J. J. |last6=Lourenço |first6=C. |last7=Masoni |first7=A. |last8=Mikhasenko |first8=M. |last9=Mitchell |first9=R. E. |last10=Patrignani |first10=C. |last11=Schwanda |first11=C. |last12=Spanier |first12=S. |last13=Venanzoni |first13=G. |last14=Yuan |first14=C. Z. |last15=Agashe |first15=K. |date=2024-08-01 |title=Review of Particle Physics |url=https://link.aps.org/doi/10.1103/PhysRevD.110.030001 |journal=Physical Review D |language=en |volume=110 |issue=3 |page=030001 |doi=10.1103/PhysRevD.110.030001 |issn=2470-0010|hdl=20.500.11850/695340 |hdl-access=free }}</ref>{{rp|25.1.1}}