2,977 research outputs found
Unconstrained Astrometric Orbits for Hipparcos Stars with Stochastic Solutions
A considerable number of astrometric binaries whose positions on the sky do
not obey the standard model of mean position, parallax and linear proper
motion, were observed by the Hipparcos satellite. Some of them remain
non-discovered, and their observational data have not been properly processed
with the more adequate astrometric model that includes nonlinear orbital
motion. We develop an automated algorithm based on "genetic optimization", to
solve the orbital fitting problem with no prior information about the orbital
elements is available (from, e.g., spectroscopic data or radial velocity
monitoring). We test this method on Hipparcos stars with known orbital
solutions in the catalog, and further apply it to stars with stochastic
solutions, which may be unresolved binaries. At a confidence level of 99%,
orbital fits are obtained for 65 stars, most of which have not been known as
binary. A few of the new probable binaries with A-type primaries with periods
444-2015 d are chemically peculiar stars, including Ap and \lambda Boo type.
The anomalous spectra of these stars are explained as admixture of the light
from the unresolved, sufficiently bright and massive companions. We estimate
the apparent orbits of four stars which have been identified as members of the
300 Myr-old UMa kinematic group. Another four new nearby binaries may include
low-mass M-type or brown dwarf companions. Similar astrometric models and
algorithms can be used for binary stars and planet hosts observed by SIM
PlanetQuest and Gaia
The case for reshoring and nearshoring as a sustainability enhancer - perspectives from the textile industry
Sustainability awareness has increased worldwide, but implementation is faltering. The
objective of the study is to find out if nearshoring is being used by textile companies to
improve their sustainability performance. Moreover, the study aims at understanding the
willingness of customers to pay more for nearshored products. To gain better insights four
expert interviews were conducted and a questionnaire was filled out by 203 people. Findings
resulting from the research indicate that nearshoring has no clear influence on sustainability
performance. Furthermore, even customers who are aware of sustainability are not willing to
spend significantly more for a sustainably produced T-shirt
HIPPARCOS Astrometric Orbit and Evolutionary Status of HR 6046
The previously known, 6-yr spectroscopic binary HR 6046 has been speculated
in the past to contain a compact object as the secondary. A recent study has
re-determined the orbit with great accuracy, and shown that the companion is an
evolved but otherwise normal star of nearly identical mass as the primary,
which is also a giant. The binary motion was detected by the Hipparcos mission
but was not properly accounted for in the published astrometric solution. Here
we use the Hipparcos intermediate data in combination with the spectroscopic
results to revise that solution and establish the orbital inclination angle for
the first time, and with it the absolute masses M(A) = 1.38 [-0.03,+0.09]
M(Sun) and M(B) = 1.36 [-0.02,+0.07] M(Sun). Aided by other constraints, we
investigate the evolutionary status and confirm that the primary star is
approaching the tip of the red-giant branch, while the secondary is beginning
its first ascent.Comment: To appear in The Astronomical Journal. 8 pages including tables and
figures, in emulateapj forma
Projet de mise en oeuvre d'un équipement d'étude et de surveillance sur le volcan Lombenben (île d'Aoba-République du Vanuatu) = Proposal for the installation of monitoring equipment on the volcano Lombenben (Ambae island, Republic of Vanuatu)
Ce rapport rassemble les principales informations qui ont justifiées la demande de mise sous surveillance de la zone sommitale du volcan Lombenben sur l'île d'Aoba (environ 10 000 habitants). Il fait état de quelques données récentes et décrit l'ensemble des travaux qui seront conduits dans les prochains mois. (Résumé d'auteur
Analysis of the eclipsing binaries in the LMC discovered by OGLE: Period distribution and frequency of the short-period binaries
We review the results of our analysis of the OGLE LMC eclipsing binaries
(Mazeh, Tamuz & North 2006), using EBAS -- Eclipsing Binary Automated Solver,
an automated algorithm to fit lightcurves of eclipsing binaries (Tamuz, Mazeh &
North 2006).
After being corrected for observational selection effects, the set of
detected eclipsing binaries yielded the period distribution and the frequency
of all LMC short-period binaries, and not just the eclipsing systems.
Somewhat surprisingly, the period distribution is consistent with a flat
distribution in log P between 2 and 10 days. The total number of binaries with
periods shorter than 10 days in the LMC was estimated to be about 5000. This
figure led us to suggest that (0.7 +- 0.4)% of the main-sequence A- and B-type
stars are found in binaries with periods shorter than 10 days. This frequency
is substantially smaller than the fraction of binaries found by small Galactic
radial-velocity surveys of B stars.Comment: 6 pages, 2 figures, submitted to Conference Proceedings of IAU Symp.
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Present teaching stories as re-membering the humanities
he ways in which Humanities scholars talk about teaching tell something about how we interact with the past of our own discipline as well as anticipate our students’ futures. In this we express collective memories as truths of learning and teaching. As cultural artifacts of our present, such stories are worthy of excavation for what they imply about ourselves as well as messages they pass onto our successors. This paper outlines “collective re-membering” as one way to understand these stories, particularly as they present in qualitative interviews commonly being used to research higher education practice in the Humanities. It defines such collective re-membering through an interweaving of Halbwachs, Ricoeur, Wertsch and Bakhtin. It proposes that a dialogic reading between this understanding of collective re-membering and qualitative data-sets enables us to both access our discursive tendencies within the Humanities and understand the impact they might have on student engagement with our disciplines, noting that when discussing learning and teaching, we engage in collectively influenced myth-making and hagiography. The paper finishes by positing that the Humanities need to change their orientation from generating myths and pious teaching sagas towards the complex and ultimately more intellectually satisfying, articulation of learning and teaching parables
On the derivation of radial velocities of SB2 components: a "CCF vs TODCOR" comparison
The radial velocity (RV) of a single star is easily obtained from
cross-correlation of the spectrum with a template, but the treatment of
double-lined spectroscopic binaries (SB2s) is more difficult. Two different
approaches were applied to a set of SB2s: the fit of the cross-correlation
function with two normal distributions, and the cross-correlation with two
templates, derived with the TODCOR code. It appears that the minimum masses
obtained through the two methods are sometimes rather different, although their
estimated uncertainties are roughly equal. Moreover, both methods induce a
shift in the zero point of the secondary RVs, but it is less pronounced for
TODCOR. All-in-all the comparison between the two methods is in favour of
TODCOR.Comment: 5 pages, 4 figures, SF2A Conference 201
The Galactic disk mass-budget : II. Brown dwarf mass-function and density
In this paper, we extend the calculations conducted previously in the stellar
regime to determine the brown dwarf IMF in the Galactic disk. We perform Monte
Carlo calculations taking into account the brown dwarf formation rate, spatial
distribution and binary fraction. Comparison with existing surveys seems to
exclude a power-law MF as steep as the one determined in the stellar regime
below 1 \msol and tends to favor a more flatish behaviour. Comparison with
methane-dwarf detections tends to favor an eventually decreasing form like the
lognormal or the more general exponential distributions determined in the
previous paper. We calculate predicting brown dwarf counts in near-infrared
color diagrams and brown dwarf discovery functions. These calculations yield
the presently most accurate determination of the brown dwarf census in the
Galactic disk. The brown dwarf number density is comparable to the stellar one,
pc. The corresponding brown dwarf mass
density, however, represents only about 10% of the stellar contribution, i.e.
\rho_{BD}\simle 5.0\times 10^{-3} \mvol. Adding up the local stellar density
determined previously yields the density of star-like objects, stars and brown
dwarfs, in the solar neighborhood \rho_\odot \approx 5.0\times 10^{-2} \mvol.Comment: 39 pages, Latex file, uses aasms4.sty, to be published in ApJ,
corrected version with correct figure
A possible dividing line between massive planets and brown-dwarf companions
Brown dwarfs are intermediate objects between planets and stars. The lower
end of the brown-dwarf mass range overlaps with the one of massive planets and
therefore the distinction between planets and brown-dwarf companions may
require to trace the individual formation process. We present results on new
potential brown-dwarf companions of Sun-like stars, which were discovered using
CORALIE radial-velocity measurements. By combining the spectroscopic orbits and
Hipparcos astrometric measurements, we have determined the orbit inclinations
and therefore the companion masses for many of these systems. This has revealed
a mass range between 25 and 45 Jupiter masses almost void of objects,
suggesting a possible dividing line between massive planets and sub-stellar
companions.Comment: 4 pages, 3 figures, submitted to IAUS 276 conference proceeding
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