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An investigation of low-mass-ratio EW systems from the Catalina Sky Survey
(SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST, 2020)
We have conducted a survey of overcontact binary systems (EW) with mass ratio <= 0.25 from the Catalina Sky Survey (CSS) that are considered strong merger candidates and are probable progenitors of FK Com-type stars and ...
Optimal sampling for repeated binary measurements
(CANADIAN JOURNAL STATISTICS, 2004)
The authors consider the optimal design of sampling schedules for binary sequence data. They propose an approach which allows a variety of goals to be reflected in the utility function by including deterministic sampling ...
BINARIES AMONG DEBRIS DISK STARS
(2012-02-01)
We have gathered a sample of 112 main-sequence starswith known debris disks.We collected published information
and performed adaptive optics observations at Lick Observatory to determine if these debris disks are ...
Resonant Raman scattering background in XRF spectra of binary samples
(Pergamon-Elsevier Science Ltd, 2015-02)
In x-ray fluorescence analysis, spectra present singular characteristics produced by the different scattering processes. When atoms are irradiated with incident energy lower and close to an absorption edge, scattering peaks ...
Stellar multiplicity and debris discs: an unbiased sample
(Oxford University Press, 2015)
Circumstellar dust discs have been observed around many nearby stars. However, many
stars are part of binary or multiple stellar systems. A natural question arises regarding the
presence and properties of such discs in ...
Formation of close binaries by triple dynamics in the context of supernovae la progenitors
(Universidad de Valparaíso, 2018-07)
The unique capabilities of Type Ia Supernovae (SN Ia), with emission bright and uniform enough to serve as yardsticks on cosmological distance scales, has resulted in them becoming some of the most important objects in the ...