1. [1] A. Einstein and E. G. Straus, '' The Influence of the Expansion of Space on the Gravitation Fields Surrounding the Individual Stars,'' Rev. Mod. Phys., vol. 17, no. 2, 1945. [
DOI:10.1103/RevModPhys.17.120]
2. [2] M. Carrera and D. Giulini, "Influence of global cosmological expansion on local dynamics and kinematics," Rev. Mod. Phys., vol. 82, no. 169, 2010. [
DOI:10.1103/RevModPhys.82.169]
3. [3] G. C. McVittie, "The mass-particle in an expanding universe," Mon. Not. R. Astr. Soc., vol. 93, no. 325, 1933. [
DOI:10.1093/mnras/93.5.325]
4. [4] B. C. Nolan, "A point mass in an isotropic universe: Existence, uniqueness, and basic properties," Phys.Rev. D, vol. 58, no. 064006, 1998. [
DOI:10.1103/PhysRevD.58.064006]
5. [5] B. C. Nolan, "A point mass in an isotropic universe: III. The region R ≤ 2m," lass.Quant.Grav., vol.16, no. 3191, 1999. [
DOI:10.1088/0264-9381/16/10/310]
6. [6] I. D. Karachentsev, "The Local Group and Other Neighboring Galaxy Groups," The Astronomical Journal, vol. 129, no. 178, 2005. [
DOI:10.1086/426368]
7. [7] B. Senevirathne and N. de Silva, "The Merger of the Schwarzschild metric and the Robertson-Walker metric," arXiv: 0812.3740v2.