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Astron. Astrophys. 329, L17-L19 (1998)

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3. Conclusion

Thus our conclusion is that the standard model with [FORMULA], [FORMULA] is ruled out, some low-density open models are possible, but the preferred range is around [FORMULA] [FORMULA], [FORMULA] and the flat geometry of Eq. (1) is possible.

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© European Southern Observatory (ESO) 1998

Online publication: November 24, 1997
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