Abstract
Large-scale inhomogeneity of the velocity field in the Perseus spiral arm region is found on the basis of the analysis of spatial motions of supergiants. The inhomogeneity seems to be connected with both presence of large groups of young stars and systematic motions in the arm predicted by the density wave theory. Proper motions of 78 stars are presented.
Gerasimenko, T P
[1]
- Ural'skij Gosudarstvennyj Univ., Sverdlovsk (USSR)
Citation Formats
Gerasimenko, T P.
Kinematic properties of supergiants in the Perseus spiral arm.
USSR: N. p.,
1963.
Web.
Gerasimenko, T P.
Kinematic properties of supergiants in the Perseus spiral arm.
USSR.
Gerasimenko, T P.
1963.
"Kinematic properties of supergiants in the Perseus spiral arm."
USSR.
@misc{etde_5424216,
title = {Kinematic properties of supergiants in the Perseus spiral arm}
author = {Gerasimenko, T P}
abstractNote = {Large-scale inhomogeneity of the velocity field in the Perseus spiral arm region is found on the basis of the analysis of spatial motions of supergiants. The inhomogeneity seems to be connected with both presence of large groups of young stars and systematic motions in the arm predicted by the density wave theory. Proper motions of 78 stars are presented.}
journal = []
volume = {9:5}
journal type = {AC}
place = {USSR}
year = {1963}
month = {May}
}
title = {Kinematic properties of supergiants in the Perseus spiral arm}
author = {Gerasimenko, T P}
abstractNote = {Large-scale inhomogeneity of the velocity field in the Perseus spiral arm region is found on the basis of the analysis of spatial motions of supergiants. The inhomogeneity seems to be connected with both presence of large groups of young stars and systematic motions in the arm predicted by the density wave theory. Proper motions of 78 stars are presented.}
journal = []
volume = {9:5}
journal type = {AC}
place = {USSR}
year = {1963}
month = {May}
}