13,120 research outputs found
Atmospheric composition of weak G band stars: CNO and Li abundances
We determined the chemical composition of a large sample of weak G band stars
-- a rare class of G and K giants of intermediate mass with unusual abundances
of C, N, and Li. We have observed 24 weak G band stars with the 2.7 m Harlan J.
Smith Telescope at the McDonald Observatory and derived spectroscopic
abundances for C, N, O, and Li, as well as for selected elements from Na - Eu.
The results show that the atmospheres of weak G band stars are highly
contaminated with CN-cycle products. The C underabundance is about a factor of
20 larger than for normal giants and the C/C ratio approaches the
CN-cycle equilibrium value. In addition to the striking CN-cycle signature the
strong N overabundance may indicate the presence of partially ON-cycled
material in the atmospheres of the weak G band stars. The exact mechanism
responsible for the transport of the elements to the surface has yet to be
identified but could be induced by rapid rotation of the main sequence
progenitors of the stars. The unusually high Li abundances in some of the stars
are an indicator for Li production by the Cameron-Fowler mechanism. A
quantitative prediction of a weak G band star's Li abundance is complicated by
the strong temperature sensitivity of the mechanism and its participants. In
addition to the unusual abundances of CN-cycle elements and Li we find an
overabundance of Na that is in accordance with the NeNa chain running in
parallel with the CN-cycle. Apart from these peculiarities the element
abundances in a weak G band star's atmosphere are consistent with those of
normal giants.Comment: 18 pages, 18 figures, accepted for publication in Ap
Nebula around R Corona Borealis
The star R Corona Borealis (R CrB) shows forbidden lines of [O II], [N II],
and [S II] during the deep minimum when the star is fainter by about 8 to 9
magnitudes from normal brightness, suggesting the presence of nebular material
around it. We present low and high spectral resolution observations of these
lines during the ongoing deep minimum of R CrB, which started in July 2007.
These emission lines show double peaks with a separation of about 170 km/s. The
line ratios of [S II] and [O II] suggest an electron density of about 100
cm. We discuss the physical conditions and possible origins of this low
density gas. These forbidden lines have also been seen in other R Coronae
Borealis stars during their deep light minima and this is a general
characteristic of these stars, which might have some relevance to their
origins.Comment: Proceedings IAU Symposium No.283, 2011 ` Planetary Nebulae: an Eye to
the Future
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Grounding semantic web services with rules
Semantic web services achieve effects in the world through web services, so the connection to those services - the grounding - is of paramount importance. The established technique is to use XML-based translations between ontologies and the SOAP message formats of the services, but these mappings cannot address the growing number of non-SOAP services, and step outside the ontological world to describe the mapping. We present an approach which draws the service's interface into the ontology: we define ontology objects which represent the whole HTTP message, and use backward-chaining rules to translate between semantic service invocation instances and the HTTP messages passed to and from the service. We present a case study using Amazon's popular Simple Storage Service
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