4,477 research outputs found
Facile Protocol for Water-Tolerant “Frustrated Lewis Pair”-Catalyzed Hydrogenation
Despite rapid advances in the field of metal-free, “frustrated Lewis pair” (FLP)-catalyzed hydrogenation, the need for strictly anhydrous reaction conditions has hampered wide-scale uptake of this methodology. Herein, we report that, despite the generally perceived moisture sensitivity of FLPs, 1,4-dioxane solutions of B(C6F5)3 actually show appreciable moisture tolerance and can catalyze hydrogenation of a range of weakly basic substrates without the need for rigorously inert conditions. In particular, reactions can be performed directly in commercially available nonanhydrous solvents without subsequent drying or use of internal desiccants
Dependence of the Fundamental Plane Scatter on Galaxy Age
The fundamental plane (FP) has an intrinsic scatter that can not be explained
purely by observational errors. Using recently available age estimates for
nearby early type galaxies, we show that a galaxy's position relative to the FP
depends on its age. In particular, the mean FP corresponds to ellipticals with
an age of ~10 Gyr. Younger galaxies are systematically brighter with higher
surface brightness relative to the mean relation. Old ellipticals form an
`upper envelope' to the FP. For our sample of mostly non-cluster galaxies, age
can account for almost half of the scatter in the B band FP. Distance
determinations based on the FP may have a systematic bias, if the mean age of
the sample varies with redshift.
We also show that fundamental plane residuals, B-V colors and Mg_2 line
strength are consistent with an ageing central burst superposed on an old
stellar population. This reinforces the view that these age estimates are
tracing the last major episode of star formation induced by a gaseous merger
event. We briefly discuss the empirical `evolutionary tracks' of
merger-remnants and young ellipticals in terms of their key observational
parameters.Comment: 14 pages, Latex, 2 figures, accepted by ApJ Letter
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