Low mass stellar companions around four giant starsYilmaz M.,
Bikmaev I.,
Sato B.,
Selam S.,
Galeev A.,
Keskin V.,
Izumiura H.,
Irtuganov E.,
Kambe E.,
Özavci I.,
Melnikov S.,
Zhuchkov R.,
Okada N. HD1695, HD120235, HD145316 and HD200004 from precise
radial velocity measurements using the 1.5 m
V1327 aquilae: A new RR lyrae variable with an extremely high radial velocity = 3.3, [M/H] = -1.05. The extremely high
radial velocity of the star's motion (V R = -470 km
Physical and dynamical parameters of the multiple system HD 222326 HD 222326. A new method for determining the individual
radial velocities of components in wide binary
Physical and dynamical parameters of the multiple system HD 222326 HD 222326. A new method for determining the individual
radial velocities of components in wide binary
V1327 aquilae: A new RR lyrae variable with an extremely high radial velocity = 3.3, [M/H] = -1.05. The extremely high
radial velocity of the star's motion (V R = -470 km
The mass of the compact object in the X-ray binary her X-1/HZ her.8 M⊙ and mv = 2.5 M⊙. These mass
estimates were made in a Roche model based on the observed
radial-velocity Spectral and photometric studies of the polar USNO-A2.0 0825-18396733, and that their formation is associated with an accretion stream. The spectra and
radial-velocity curves indicate
Low mass stellar companions around four giant starsYilmaz M.,
Bikmaev I.,
Sato B.,
Selam S.,
Galeev A.,
Keskin V.,
Izumiura H.,
Irtuganov E.,
Kambe E.,
Özavci I.,
Melnikov S.,
Zhuchkov R.,
Okada N. HD1695, HD120235, HD145316 and HD200004 from precise
radial velocity measurements using the 1.5 m
Новые конструкции и методы оценки точности планетарных радиально-плунжерных передачСасковец, К. В.,
Капитонов, А. В.,
Лебедев, М. В.,
Saskovets, K. V.,
Kapitonov, A. V.,
Lebedev, M. V. New designs and computer models for Siemens NX planetary
radial plunger transmissions with iproved