Results 161 to 170 of about 1,546,467 (200)
Rotationally Resolved Predissociation Spectrum of the 1<sup>5</sup>Φ ← X<sup>5</sup>Δ Rovibronic Band of FeH. [PDF]
Jin S +4 more
europepmc +1 more source
Counting Cosmic Cycles: Past Big Crunches, Future Recurrence Limits, and the Age of the Quantum Memory Matrix Universe. [PDF]
Neukart F, Marx E, Vinokur V.
europepmc +1 more source
Strong gravitational lenses from the Vera C. Rubin Observatory. [PDF]
Shajib AJ +8 more
europepmc +1 more source
On the Coupling Between Cosmological Dynamics and Quantum Behavior: A Multiscale Thermodynamic Framework. [PDF]
Warkentin A.
europepmc +1 more source
Evidence for the first globular cluster stellar stream beyond the Milky Way. [PDF]
Holm JK +7 more
europepmc +1 more source
Nonlinear stability and vibration of flexible spacecraft solar arrays under thermally induced flutter during the penumbra phase. [PDF]
Motaharifard O +2 more
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Considerable progress has been made in determining the Hubble constant over the past two decades. We discuss the cosmological context and importance of an accurate measurement of the Hubble constant, focusing on six high-precision distance-determination ...
Barry F. Madore, Wendy Freedman
exaly +4 more sources
A buyer’s guide to the Hubble constant [PDF]
AbstractSince the expansion of the universe was first established by Edwin Hubble and Georges Lemaître about a century ago, the Hubble constant $$H_0$$ H 0 which measures its rate has been of great interest to astronomers. Besides being interesting in its own
Ofer Lahav, Pablo Lemos, Paul Shah
exaly +4 more sources
An analytical method to calculate Hubble’s constant [1] is presented. The proposed procedure is an alternative scheme to the red shifts of spectral lines picture, to obtain the value of that constant [2].
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Science, 1992
The Hubble constant is the constant of proportionality between recession velocity and distance in the expanding universe. It is a fundamental property of cosmology that sets both the scale and the expansion age of the universe. It is determined by measurement of galaxy radial velocities and distances.
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The Hubble constant is the constant of proportionality between recession velocity and distance in the expanding universe. It is a fundamental property of cosmology that sets both the scale and the expansion age of the universe. It is determined by measurement of galaxy radial velocities and distances.
openaire +2 more sources

