A machine learning method for predicting telescope cycle time applied to the Cerro Murphy Observatory. [PDF]
Kicia M +4 more
europepmc +1 more source
Female intuition in economics and conscious leadership: a comprehensive integrative review of conceptual foundations, cultural moderators, and future directions. [PDF]
Gómez Tobías R.
europepmc +1 more source
Geneticization in the genomic era: a scoping review of ethical, clinical, and sociocultural transformations. [PDF]
Shaheen S, Ghaly M.
europepmc +1 more source
The Reflection Effect in Eclipsing Binary Systems.
openaire +1 more source
Occupation in the Anthropocene and Ethical Relationality. [PDF]
Kiepek N.
europepmc +1 more source
Orbital and physical parameters of eclipsing binaries from the ASAS catalogue – XI. CHIRON investigation of long-period binaries [PDF]
We present the results of a spectroscopic campaign on eclipsing binaries with long orbital period (P = 20 - 75 d) carried out with the CHIRON spectrograph.
David R. Anderson +2 more
exaly +2 more sources
Ten eclipsing binaries in the Small Magellanic Cloud: fundamental parameters and Cloud distance [PDF]
We present the first results of an observational programme to measure the fundamental parameters of over 100 eclipsing binaries in the Small Magellanic Cloud (SMC).
Timothy Harries +2 more
exaly +1 more source
Related searches:
A Millisecond Pulsar in an Eclipsing Binary
Nature, 1988We report the discovery of a remarkable pulsar with period 1.6 ms, moving in a nearly circular 9.17 hour orbit around a low mass companion star. At an observing frequency of 430 MHz, the pulsar, PSR 1957+20, is eclipsed once each orbit for about 50 minutes.
A. S. Fruchter +2 more
openaire +1 more source
The Eclipsing Binary WX Eridani
International Astronomical Union Colloquium, 1979AbstractThe Algol-type eclipsing binary WX Eridani was observed on 21 nights on the 48-inch telescope of the Japal-Rangapur Observatory during 1973-75 in B and V colours. An improved period of P = 0.82327038 days was obtained from the analysis of the times of five primary minima.
M. B. K. Sarma, K. D. Abhyankar
openaire +1 more source
AB Andromedae – An overcontact eclipsing binary
New Astronomy, 2021Abstract In an effort to resolve the discrepancy between two earlier studies, new radial velocity and photometric data have been obtained and analyzed by Roche modelling for AB Andromedae, an overcontact W-subtype eclipsing binary. The new values for the basic data, m1 = 0.60 (3) Mʘ, m2 = 1.14 (3) Mʘ, R1 = 0.81 (1) Rʘ, R2 = 1.08 (1) Rʘ, L1 = 0.73 (6)
openaire +2 more sources

