# The Cosmic Microwave Background and Observational Convergence in the Ω[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF]-Ω[TINF]Λ[/TINF] Plane

@article{Lineweaver1998TheCM, title={The Cosmic Microwave Background and Observational Convergence in the $\Omega$[TINF][CLC][ITAL]m[/ITAL][/CLC][/TINF]-$\Omega$[TINF]$\Lambda$[/TINF] Plane}, author={C. Lineweaver}, journal={The Astrophysical Journal}, year={1998}, volume={505}, pages={L69-L73} }

I use the most recent cosmic microwave background (CMB) anisotropy measurements to constrain the leading cold dark matter models in the Omega_m - Omega_lambda plane. A narrow triangular region is preferred. This triangle is elongated in such a way that its intersection with even conservative versions of recent supernovae, cluster mass-to-light ratios and double radio source constraints, is small and provides the current best limits in the Omega_m - Omega_lambda plane: Omega_lambda = 0.62 +/- 0…

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