Interstellar cloud morphologies and their origins

Articles in the same Issue

1. Titelei
2. Contents
3. Preface
4. List of Participants
5. Astronomy at the Vilnius University
6. The transition between stellar populations in the Galaxy
7. HIPPARCOS programme for field metal-deficient F-M stars
8. Catalogues of field Population II stars
9. Progress report on the radial velocity measurement programme of Population II stars
10. A set of standards for stellar classification of metaldeficient stars in the Vilnius system
11. Ultraviolet intrinsic colour indices of O- and B-type stars
12. The microchannel plate intensifier for intensified CCD photon-counting systems
13. Stellar evolution on the asymptotic giant branch: some actualities
14. Interstellar cloud morphologies and their origins
15. The accuracy of stellar metal abundances from intercomparison of catalogues
16. Element abundances in planetary nebulae from recombination line spectra
17. On the validity of the exponential size distribution function of interstellar dust
18. Theoretical atomic data for astrophysics
19. The epochs of bulge and disk formation
20. Dust formation in supernova ejecta
21. A project for investigation of stellar population of the galactic disk
22. Intrinsic colour indices of O- and B-type stars in the Vilnius photometric system
23. Red horizontal branch stars in the galactic field
24. The mass-to-light ratio of the visible matter
25. Dissipative evolution of protogalactic cloud systems
26. A computer program for two-dimensional quantification of normal stars in the Vilnius photometric system