FRACTALITY AND KINETICS OF THE STELLAR MEDIUM IN THE SOLAR NEIGHBORHOOD BASED ON GAIA DR2 DATA
Section: STARS AND THE INTERSTELLAR MEDIUM
Authors:
1.
Sternberg State Astronomical Institute of Moscow State
University
2.
Sternberg State Astronomical Institute of Moscow State
University
Physical Faculty of Moscow State University
Russian Federation
Physical Faculty of Moscow State University
Russian Federation
Type:
Сonference article
Published:
27.12.2024
Subject area:
52
53
520
521
523
524
52-1
52-6
41.00
29.35
29.31
29.33
29.27
29.05
03.06.01
03.05.01
03.04.03
2
223
614
6135
SCI004000
SCI005000
53
520
521
523
524
52-1
52-6
41.00
29.35
29.31
29.33
29.27
29.05
03.06.01
03.05.01
03.04.03
2
223
614
6135
SCI004000
SCI005000
Language:
English
Keywords:
Galaxy: evolution, solar neighborhood, structure; stars: kinematics and dynamics
Abstract (English):
The fractal nature of the stellar medium in the Solar vicinity has been established by studying 200 000 stars of all spectral types at distances of 1 to 100 parsec from the Sun. The fractal dimension is
The fractal nature of the stellar medium in the Solar vicinity has been established by studying 200 000 stars of all spectral types at distances of 1 to 100 parsec from the Sun. The fractal dimension is
Keywords:
Galaxy: evolution, solar neighborhood, structure; stars: kinematics and dynamics
Galaxy: evolution, solar neighborhood, structure; stars: kinematics and dynamics
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