CiteSeerX — Table search results

Results 1 - 10 of 11,049

Table 3. Elemental abundance ratios in V854 Cen compared to predictions from s-processing calculations for di erent neutron exposures 0

by Martin Asplund, Bengt Gustafsson, N. Kameswara Rao, David L. Lambert

Table 8. Abundances of s-process elements in CH stars, barium stars and normal giant stars belonging to a barium-like binary system. The column labeled `elements apos; lists the elements involved in [s/Fe]. Usually [s/Fe] = 0.5 ([Y/Fe] + [Nd/Fe]); YII/TiII in that column means that [s/Fe] corresponds to the [Y/Ti] ratio taken from McWilliam (1990; see Appendix for details). The column labeled `Ref apos; provides the reference for the [s/Fe] data, according to the notes at the end of the table. The orbital periods of CH systems are from McClure amp; Woodsworth (1990) a. CH stars

in Insights into the formation of barium and Tc-poor S stars from an extended sample of orbital elements

by Jorissen Van Eck, A. Jorissen, M. Mayor, S. Udry

"... In PAGE 12: ...88, (38 ? 41) = ?0:20, K4Ba5), both ana- lyzed by Smith (1984). Despite very di erent orbital pe- riods, the level of chemical peculiarities in these two stars is similar, as indicated not only by their heavy-element overabundances ( Table8 ) but also by their uorine abun- dance (Jorissen et al. 1992a).... In PAGE 12: ...ig. 7. Their very existence is another clear indication that the orbital separation is not the only parameter controlling the level of chemical peculiarities in barium stars. These barium-like binary systems involving a normal giant are listed in Table8 and are collected from the catalogue of Bo n et al. (1993), listing all spectroscopic binary systems with a giant component.... In PAGE 12: ... 7. Orbital period vs heavy-element overabundance [s/Fe] (see Table8 ). Filled dots correspond to barium and normal giants in barium-like binary systems, whereas open dots corre- spond to CH stars.... ..."

Table 4. Summary of mapping between FBPML and OWL-S process primitives Primitive FBPML OWL-S

in Translating a Typical Business Process Modelling Language to a Web Services Ontology through Lightweight Mapping

by Gayathri Nadarajan, Yun-heh Chen-burger

"... In PAGE 15: ... A precise specification of what it means to perform a process in OWL-S has not been given yet. Table4 summarises the mapping of the primitives between FBPML PL and OWL-S process ontology. 6.... In PAGE 22: ... 15: End the OWL file (enclose with lt;/rdf:RDF gt; tag). Or, time points and synchronisation of time points (See Table4 ). The implications of such missing elements could be severe from a business processing point of view.... ..."

Table 1: Time of invocation using the centralized method of argument transfer: m is the number of server apos;s processes, n is the number of client apos;s processes, the time is given in milliseconds.

in PARDIS: A Parallel Approach to CORBA

by Katarzyna Keahey, Dennis Gannon 1997

"... In PAGE 9: ... Since it is likely that invocations on SPMD objects will most often involve transferring large arguments, we will concentrate on evaluating the e ciency of this method for a relatively large sequence composed of 217 of elements of type double. Table1 summarizes the results.... ..."

Cited by 39

Table 1. Summary of the Modeling of OWL-S Process Models in Promela .

in Towards a Formal Verification of OWL-S Process Models

by Anupriya Ankolekar, Massimo Paolucci, Katia Sycara

"... In PAGE 12: ...2 Summary of the OWL-S Model construction This section presented a detailed description of the modeling of OWL-S Process Models in the Promela modeling language. A summary of our modeling is presented in Table1 , highlighting the OWL-S Process Model features retained, partially modeled and the features out of scope. We already discussed how the checking of data values could be deferred to a type-checker or semantic reasoner.... ..."

Cited by 1

Table 1. Relative r and s contributions to some elements in the Solar System Element log N s-weak s-main r

in Galactic chemical evolution of primary elements in the solar neighbourhood II: Elements affected by the s-process

by Pagel And, G. Tautvaisiene

"... In PAGE 3: ... The r- process contribution to each element can now be judged either according to solar-system data (Cameron 1982; Kappeler, Beer amp; Wisshak 1989) or according to the de- ciency found relative to Eu or Dy in that star, with rea- sonably good agreement. Relevant numbers are shown in Table1 , where we list relative contributions from the weak and main s-processes and from the r-process according to solar-system data after Kappeler, Beer amp; Wisshak (1989) updated by Raiteri, Gallino amp; Busso (1992), the resulting de ciency relative to europium in a pure r-process and the corresponding de ciencies ac- tually found in CS 22892-052 by Sneden et al. (1996).... In PAGE 4: ... 3 SEPARATING R AND S-PROCESS CONTRIBUTIONS To visualize the development of r and s-process contribu- tions to the various elements of interest, we show in Fig 1 the data for element ratios relative to europium, taken as representative of a virtually pure r-process. As expected, most elements with a large s-process contribution according to Table1 show a progressive increase from somewhere near the pure r-process ratio to the solar-system ratio at [Fe/H] = 0. Furthermore, the typical \s-process quot; elements Sr, Y, Ba, La and Ce seem to de ne a plateau between [Fe/H] = ?2:1 and ?0:5 (cf.... In PAGE 6: ... (1995) (asterisks). The large open square shows the r-process ratio predicted from Solar System data according to Table1 and the black 5-pointed star the corresponding ratio from CS 22892-052. Table 3.... ..."

Table 1. {Continued}

in Model Transformation from OWL-S to BPEL Via

by Behzad Bordbar, Gareth Howells, Michael Evans, Athanasios Staikopoulos

"... In PAGE 10: ... Bordbar et al. Table1 . Equivenlent mapping of OWL-S Process and BPEL elements OWL-S Process BPEL lt;Process gt; lt;Process gt; lt;AtomicProcess gt; lt;Process gt; + lt;PortType gt; + lt;Operation gt; + lt;PartnerLinkType gt; + lt;Role gt; + lt;invoke gt; Operation + PortType names must be consis- tent with the created WSDL file.... ..."

Table 1: The s{process calculations with a parametrized model (SP model)a to check the in uence of the MAC cross sections BP of the branch point isotopes on the s{process neutron density nn and temperature kT . Branch point isotopes

in Neutron Capture Reaction Rates of Unstable Isotopes in the s--Process Branchings

by Rauscher Beer, Forschungszentrum Karlsruhe

"... In PAGE 2: ... The experimental values for the stable isotopes were supplemented by our newly deter- mined theoretical rates. The neutron densities and temperatures obtained in the SP model (pulsed s-process; burning of one neutron source) [10] are given in Table1 . The quoted errors arise mainly from an estimate of the average deviation of the theoretical cross sections compared to experimental data, as mentioned above.... ..."

Table 2: Time of invocation using the multi-port method of argument transfer: m is the number of server apos;s processes, n is the number of client apos;s processes, the time is given in milliseconds.