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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Molecular genetics and genomics 255 (1997), S. 410-419 
    ISSN: 1617-4623
    Keywords: Key words Meiosis ; Yeast ; Intron ; Recombination ; Splicing
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract REC114 is one of 10 genes known to be required for the initiation of meiotic recombination in Saccharomyces cerevisiae. It is transcribed only in meiosis, and our previous sequence analysis suggested the presence of an intron in the 3′ end of the gene. Hypotheses in the literature have suggested, because of its unusual location, either that the putative intron in REC114 is likely to be necessary for expression, or that there may actually be no intron present. This work demonstrates that REC114 does have an intron and is one of only three genes in yeast with introns located in the 3′ end. Furthermore, the 3′ splice site utilized in REC114 is a very rare AAG sequence; only three other genes in yeast use this nonconsensus sequence. The splicing of REC114 does not require MER1, a gene known to be involved in meiosis-specific RNA processing. In fact, an intronless copy of REC114 can complement a null rec114 mutation. Thus, it does not appear that the intron is essential for expression of REC114. Although the intron is not absolutely required for meiotic function, it is conserved in evolution; two other species of yeast contain an intron at the same location in their REC114 genes.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-06-28
    Description: Detailed numerical calculations which are solutions of the full set of general relativistic equations describing the evolution of a spherical star are presented, for the case of the evolution of neutron stars that are cooling over the central temperatures range of 10 to the 10th to 10 to the 7th K. The effects of nucleon superfluidity in the inner crust and core are included, and models are constructed with and without a pion condensate at high densities. It is found that the localized neutrino cooling which dominates the early evolution of neutron stars is so rapid that heat transport within the star cannot keep pace, and temperature distribution is not isothermal. The residual contraction of the neutron star during the early cooling phase contributes little to the heat budget of the star, and most of the gravitational energy released raises the Fermi energy of the degenerate nucleons. It is concluded that since calculations with and without pion condensate are consistent with the upper limits of current observations, these are not sufficient in distinguishing between the various models of neutron star cooling.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal; vol. 255
    Format: text
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