You are seeing reference results for evolutionary mass because there's not a match on Dictionary.com.
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www.reference.com/topic/Evolutionary-Stage-of-Stars
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Astronomers believe that white dwarf stars are the final evolutionary stage of stars with roughly the mass of the Sun. For the majority of its life, a solar mass star is in the main sequence
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www.bizplenty.com/State_of_Ohio_IRS
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Further, if the two stars have the same mass and evolutionary state, then there should be no systemic color change over the period; as mentioned above, this is contrary to the obse...
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www.reference.com/topic/Explain-the-Mechanisms-That-Lea...
www.reference.com/topic/Explain-the-Mechanisms-That-Lead-to-Evolutionary-Change
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STANDARDS: A. (Max 7 points) Explain the mechanisms that lead to evolutionary change. The Big Picture: (1 point for any of the following) __ Punctuated Equilibrium, mass extinction, etc.
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Jan 9, 2008 ... Abstract: I investigate the discrepancy between the evolution and pulsation masses for Cepheid variables. A number of recent works have ...
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iopscience.iop.org/0004-637X/629/2/1021/61791.text.html
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In the last decades, a large amount of work has been devoted to the comparison between pulsation and evolutionary masses, leading to the long-debated ...
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iopscience.iop.org/0004-637X/677/1/483/73442.text.html
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Cepheid Mass Loss and the Pulsation-Evolutionary Mass Discrepancy ... I investigate the discrepancy between the evolution and pulsation masses for Cepheid ...
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iopscience.iop.org/0004-637X/629/2/1021/pdf/61791.web.p...
iopscience.iop.org/0004-637X/629/2/1021/pdf/61791.web.pdf
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the evolution of intermediate-mass stars and, in particular, the occurrence of ... parison with evolutionary masses Me;can inferred by canonical. (i.e., no mass ...
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adsabs.harvard.edu/abs/1986Ap%26SS.128..319T
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Title: Population I pulsating stars. III - Period-Evolutionary mass(-colour) relations. Authors: Tsvetkov, Ts. G. Affiliation: AA(Sofiiski Universitet, Sofia, Bulgaria) ...
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www.sciencedaily.com/releases/2012/02/120213154055.htm
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8 hours ago ... Fossil record of graptoloids challenges the theory that immediately after a mass extinction, species develop new physical traits at a rapid pace.
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www.eso.org/public/archives/releases/sciencepapers/eso1...
www.eso.org/public/archives/releases/sciencepapers/eso1046/eso1046.pdf
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mass determination for a classical Cepheid variable star (as opposed to type-II Cepheids, low-mass stars with a very different evolutionary history) in a binary ...
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