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20022026
most citedThe Milky Way Spiral Structure Parameters from Data on Masers and Selected Open Clusters

73 citations · 1.2k across the 109 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 40 cited

Galactic Rotation Curve and the Effect of Density Waves from Data on Young Objects

V. V. Bobylev, A. T. Bajkova, A. S. Stepanishchev

Based on currently available data on the three-dimensional field of space velocities of young (<50 Myr) open star clusters and the radial velocities of HI clouds and star-forming (…

astro-ph2007★ 14 cited

Spectral Spatial Fluctuations of CMBR: Strategy and Concept of the Experiment

Viktor Dubrovich, Anisa Bajkova, Vladimir Khaikin

Spectral Spatial Fluctuations (SSF) of the Cosmic Microwave Background Radiation (CMBR) temperature are considered as a result of an interaction of primordial atoms and molecules w…

astro-ph2007★ 24 cited

Galactic Rotation Parameters from Data on Open Star Clusters

V. V. Bobylev, A. T. Bajkova, S. V. Lebedeva

Currently available data on the field of velocities Vr, Vl, Vb for open star clusters are used to perform a kinematic analysis of various samples that differ by heliocentric distan…

astro-ph2007★ 17 cited

Kinematics of the Scorpius-Centaurus OB Association

Vadim V. Bobylev, Anisa T. Bajkova

A fine structure related to the kinematic peculiarities of three components of the Scorpius-Centaurus association (LCC, UCL, and US) has been revealed in the UV-velocity distributi…

astro-ph2007★ 14 cited

Analysis of the Velocity Field of F and G Dwarfs in the Solar Neighborhood as a Function of Age

Vadim V. Bobylev, Anisa T. Bajkova

The space velocities from the catalog of Nordstrom et al. (2004) are used to trace variations of a number of kinematic parameters of single F and G dwarfs as a function of their ag…

astro-ph2006★ 9 cited

Investigation of Negative K-Effect Using the Osaca Catalogue

Vadim V. Bobylev, Anisa T. Bajkova, George A. Gontcharov

We created and are constantly updating the Orion Spiral Arm CAtalogue (OSACA) for stars with known coordinates, parallaxes, proper motions and radial velocities. It is shown that t…