A comprehensive understanding of the C. elegans STAR proteins GLD-1 and ASD-2 is emerging from a combination of studies. Those employing genetic analysis reveal in vivo function, others involving biochemical approaches pursue the identification of mRNA targets through which these proteins act. Lastly, mechanistic studies provide the molecular pathway of target mRNA regulation.
We show a newly found correlation of higher iron abundance in stars with
Planets (SWPs) that have binary companions that varies with period and
Eccentricity. We also present new period dependencies of the recently
Discovered correlation of stellar [Fe/H] with orbital eccentricity, which was
We will present STAR's recent dielectron measurements in the
Low and intermediate mass range for RHIC beam energies ranging between 19.6 and
200 GeV. Compared to electrons, muon measurements have the advantage of reduced
Bremsstrahlung radiation in the surrounding detector materials. With the
We study for the first time the X-ray emission of HM1 and
IC2944/2948. Low-mass, pre-main-sequence objects with an age of a few Myr are
Detected, as well as a few background or foreground objects. Most massive stars
In both clusters display the usual high-energy properties of that type of
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