Results 21 to 30 of about 75,171 (318)

An Adaptive Optics Survey of Stellar Variability at the Galactic Center [PDF]

open access: yes, 2018
We present a $\approx 11.5$ year adaptive optics (AO) study of stellar variability and search for eclipsing binaries in the central $\sim 0.4$ pc ($\sim 10''$) of the Milky Way nuclear star cluster.
Becklin, Eric E.   +11 more
core   +3 more sources

STATISTICAL RESTORATION OF SECONDARY MINIMA DEPTHS FOR ECLIPSING VARIABLE STARS AND SPECIFICATION OF THEIR EVOLUTIONARY TYPES

open access: yesOdessa Astronomical Publications, 2017
30 unknown magnitudes of secondary minima depths for eclipsing variable stars are restored by ZET - method. Evolutionary types of some eclipsing variable stars arespecified on the basis of obtained data.
E. M. Svirskaya
doaj   +1 more source

Eclipsing Binaries in Open Clusters [PDF]

open access: yes, 2006
Detached eclipsing binaries are very useful objects for calibrating theoretical stellar models and checking their predictions. Detached eclipsing binaries in open clusters are particularly important because of the additional constraints on their age and ...
B. Chaboyer   +17 more
core   +6 more sources

Parameterization of long-period eclipsing binaries

open access: yesOpen Astronomy, 2022
One of the important sources for independent determination of stellar masses is eclipsing binaries with components on the main sequence, and with observable spectral lines of both components.
Pakhomova Polina   +4 more
doaj   +1 more source

Mass-Accreting Pulsating Components of Algols

open access: yesGalaxies, 2022
We present a review of the latest results of studies of the class of mass-accreting pulsating components of semi-detached eclipsing binaries known as oEA stars.
David Mkrtichian   +5 more
doaj   +1 more source

Fundamental Properties of Late-Type Stars in Eclipsing Binaries

open access: yesGalaxies, 2022
Evidence from the analysis of eclipsing binary systems revealed that late-type stars are larger and cooler than predicted by models, and that this is probably caused by stellar magnetic activity.
Juan Carlos Morales   +3 more
doaj   +1 more source

Kepler Eclipsing Binary Stars. V. Identification of 31 Eclipsing Binaries in the K2 Engineering Data-set [PDF]

open access: yes, 2014
Over 2500 eclipsing binaries were identified and characterized from the ultra-precise photometric data provided by the Kepler space telescope. Kepler is now beginning its second mission, K2, which is proving to again provide ultra-precise photometry for ...
Abdul-Masih, Michael   +10 more
core   +3 more sources

The binary properties of the pulsating subdwarf B eclipsing binary PG 1336-018 (NY Virginis) [PDF]

open access: yes, 2007
Aims. We present an unbiased orbit solution and mass determination of the components of the eclipsing binary PG1336−018 as a critical test for the formation scenarios of subdwarf B stars. Methods. We obtained high-resolution time series VLT/UVES spectra
Al-Naimiy   +54 more
core   +9 more sources

PHOTOMETRIC OBSERVATIONS OF A NEW ECLIPSING BINARY NSVS 8213217

open access: yesOdessa Astronomical Publications, 2016
The photometric CCD observations for new suspected eclipsing binary NSVS8213217 inAstronomical stations nearOdessa(Ukraine) have been carried out. The light curves in V system were obtained and new adjusting period and light element was received.
S. N. Udovichenko
doaj   +1 more source

eclipsed (eclipsing) [PDF]

open access: yes, 2014
Citation: 'eclipsed (eclipsing)' in the IUPAC Compendium of Chemical Terminology, 3rd ed.; International Union of Pure and Applied Chemistry; 2006. Online version 3.0.1, 2019. 10.1351/goldbook.E01884 • License: The IUPAC Gold Book is licensed under Creative Commons Attribution-ShareAlike CC BY-SA 4.0 International for individual terms.
openaire   +1 more source

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