Data for Stars at One Core Radius
Physics of Stars and Measurement Data: Part I
... the stars and the Sun which was measured by astronomers is considered as a main task of the physics of ...to data of astronomical measurements: the temperature- radius-mass-luminosity relations, the ...
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Physics of Stars and Measurement Data: Part II
... binary stars 3.1 The apsidal rotation of close binary stars The apsidal rotation (or periastron rotation) of close binary stars is a result of their non-Keplerian movement which originates from the ...
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Physics of Stars and the Measurement Data: Part III
... the stars and the Sun which was measured by astronomers is considered as a main task of the physics of ...to data of astronomical measurements: the temperature-radius-mass-luminosity relations, the ...
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Investigating the A-type stars using Kepler data
... archival data, a Guest Observer program exists 3 , whereby anyone can propose to observe a target, and find the tools and documentation to make use of the ...The data processing pipelines have come under ...
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Characterizing the variability of stars with early-release Kepler data
... of data publicly released by the Kepler ...public data set (30 minute sampling and ...of stars in the ...giant stars are variable with a noise floor of ...of data set baseline (1–33 ...
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Getting to “The 5 stars of Linked Open Data” for Nanoinformatics
... available on the web (whatever format); make it available as structured data (e.g. excel instead of image scan of a table); non-proprietary format (e.g. csv instead of excel); use URL[r] ...
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RR Lyrae stars: new discoveries in the OGLE data
... Blazhko Effect in double-mode RR Lyr stars.. Chadid et al. Poretti et al. Benkö et al. Guggenberger et al. Gruberbauer et al.. Chadid et al. Poretti et al. Benkö et al. Guggenberger et a[r] ...
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One-micron spectroscopy of normal OB stars
... 3.2 Correlation with lines in the K band It is of interest to compare the behaviour of the leading IR He i Table 2. Equivalent-width measurements for major features in giant and main-sequence spectra; errors are ...
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Improved Mass and Radius Constraints for Quiescent Neutron Stars in Omega Cen and NGC 6397
... higher than the average, while the XMM-Newton/pn detec- tor measured fluxes 10% lower than the average among other detectors. Nevalainen, David & Guainazzi (2010), compar- ing Chandra/ACIS and XMM-Newton/EPIC ...
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Ike Antkare one of the great stars in the scientific firmament
... Shown in Figure 3, the first two experiments call attention to RokyTue’s instruction rate. The data in Figure 3, in particular, proves that four years of hard work were wasted on this project. Next, Gaussian ...
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An attempt to calibrate core overshooting using the seismic properties of low-mass stars
... these data by confronting them to the grid of models that was built and obtain constraints on the amount of core ...0.30. Core overshooting was included as a simple extension of the homogeneous ...
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2D dynamics of the radiative core of low mass stars
... The Ekman layer has a characteristic thickness of √ E, where we recall that E is the dimensionless Ekman num- ber. We therefore compute the averaged surface rotation rate δΩ S θ just outside of it to avoid the boundary ...
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Two-On-One Pursuit with a Non-zero Capture Radius
... REPORT DOCUMENTATION PAGE Form Approved OMB No. 0704–0188 The public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instructions, ...
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A Midpoint–Radius approach to regression with interval data
... used one is the Endpoints (EP) representation given in ...the Radius (R) coordinates are used (see ...(the radius) viewed as an upper bound of its measurement ...EP one, we refer the reader to ...
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Sensitivity and Stability Radius in Data Envelopment Analysis
... analysis, one may want to know how sensitive these identications are, for possible vari- ations in the ...which data variations will not alter a DMU ; s classication from ecient to inecient status (or vice ...
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The seismic properties of low-mass He-core white dwarf stars
... dwarf stars have composition gradients in their interiors (Althaus et ...of one or more narrow re- gions in which the abundances of nuclear species (and so, the average molecular weight μ) are spatially ...
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The Seismic Properties Of Low-Mass He-Core White Dwarf Stars
... dwarf stars have composition gradients in their interiors (Althaus et ...of one or more narrow re- gions in which the abundances of nuclear species (and so, the average molecular weight μ) are spatially ...
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All in One Core Java Faq
... Whether you use random access I/O or sequential access really depends upon what you are trying to do. Random access I/O is usually used for fixed-size data records, where you want to overwrite the original record ...
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Efficient mass estimate at the core of strong lensing galaxy clusters using the Einstein radius.
... the core mass to inform the mass –concentration relation, it is important to test whether this mass estimator introduces correlated ...the core of the ...observational data prior to a detailed SL ...
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Sails Full of Stars o a World of Adventure for Fate Core (7358435) (1)
... Dreams of Dragons This subplot is best for characters who are interested in scientific curiosities or who are merely impulsive. A peddler sells one of the PCs a pendant with a multicolored stone, on which is a ...
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