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Additive technologies in mechanical engineering

Dynamical stability of the quadruple systems HD 68255/6/7 and HD 76644 via numerical integration of the equations of motion of the four-body problem, with a chainlike

Multiple stars: Physics vs. dynamics

PHILOSOPHY AS HISTORY OF PHILOSOPHY (a round-table discussion on the book by V. V. Sokolov)PHILOSOPHY AS HISTORY OF PHILOSOPHY (a round-table discussion on the book by V. V. Sokolov)

Dynamical investigations of the multiple stars© 2017 O. V. Kiyaeva and R. Y. Zhuchkov Two multiple stars — the quadruple star Bootis (ADS 9173

Dynamical stability of the quadruple systems HD 68255/6/7 and HD 76644 via numerical integration of the equations of motion of the four-body problem, with a chainlike

Gliese 225.2: An old (stable?) quadrupletWe discovered with adaptive optics a new component E in the nearby multiple system Gliese 225

Multiple stars: Physics vs. dynamics

Physical parameters and dynamical properties of the multiple star o and that the configuration of the system is 2 + 2, where one of the subsystems is a spectral binary with a period of 33 d

V1327 aquilae: A new RR lyrae variable with an extremely high radial velocityWe have carried out photometry and spectroscopy of the star V1327 Aql (R = 16 m ) as part of our

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