Article
Open Access
Disk Galaxy Models Driven by Stochastic Self-Propagating Star Formation
-
T. Mineikis
and
V. Vansevičius
Published/Copyright:
April 19, 2017
Received: 2010-6-2
Accepted: 2010-7-1
Published Online: 2017-4-19
Published in Print: 2010-6-1
© 2017
Articles in the same Issue
- Young Stars in the Camelopardalis Dust and Molecular Clouds. VI. YSOs Verified by Spitzer and Akari Infrared Photometry
- Wide Field Multicolor CCD Photometry of the Open Cluster NGC752
- Multicolor CCD Photometry of the Open Cluster IC 361
- Chemical Composition of the RS CVn-Type Star Lambda Andromedae
- Disk Galaxy Models Driven by Stochastic Self-Propagating Star Formation
- Orthogonal Basis Functions over the Binocular Pupil
- Karhunen-Loève Basis Functions Of Kolmogorov Turbulence In The Sphere (Baltic Astronomy, 17, 383, 2008, Erratum)
Creative Commons
BY-NC-ND 4.0
Articles in the same Issue
- Young Stars in the Camelopardalis Dust and Molecular Clouds. VI. YSOs Verified by Spitzer and Akari Infrared Photometry
- Wide Field Multicolor CCD Photometry of the Open Cluster NGC752
- Multicolor CCD Photometry of the Open Cluster IC 361
- Chemical Composition of the RS CVn-Type Star Lambda Andromedae
- Disk Galaxy Models Driven by Stochastic Self-Propagating Star Formation
- Orthogonal Basis Functions over the Binocular Pupil
- Karhunen-Loève Basis Functions Of Kolmogorov Turbulence In The Sphere (Baltic Astronomy, 17, 383, 2008, Erratum)
