Non-Stable Stars

Table of Contents

Preface
Part I. Instability in Dwarf Stars of Later Type: T Tauri Stars and Related Objects, and the UV Ceti Variables:
1. On the nature and origin of the T Tauri stars George H. Herbig
2. Irregular variable stars of the RW Aurigae type P. N. Kholopov
3. On RW Aurigae type stars and related types C. Hoffmeister
4. The possible connexion between T Tauri stars and UV Ceti stars Guillermo Haro
5. Flare spectra in dwarf stars Alfred H. Joy
6. Photo-electric observations of AE Aquarii F. Lenouvel
Part II. Instability in the Hot Stars of Low Luminosity and in the Novae:
7. Evidence for instability among sub-luminous stars Jesse L. Greenstein
8. The extremely rapid light-variations of old novae and related objects Merle F. Walker
9. Physical processes in novae E. R. Mustel
10. Sub-system of novae I. M. Kopylov
11. On the causes of stellar bursts I. E. Gurevitch and A. I. Lebedinsky
12. On the nature of planetary nebulae I. S. Shklovsky
Discussion
Part III. Instability in the Luminous Stars of Early Type:
13. On the atmospheres of the Wolf-Rayet stars B. A. Vorontsov-Velyaminov
14. Instability in stars of early spectral type Otto Struve
Discussion
Part IV. Instability in the Regular Variables of Later Type:
15. Variable stars and problems of stellar formation B. V. Kukarkin
16. The stars with double envelopes V. P. Tsesevich
Part V. Phenomena of Instability in Binary Systems:
17. The instability of sub-giants in close binary systems Zdenĕk Kopal
18. Phenomena of non-stability in close binary systems D. J. Martynov
19. Photometric evidence of instability in eclipsing systems Frank Bradshaw Wood
20. Non-stability in close binary stars V. A. Krat
21. The chromospheric spectrum and the atmosphere of 31 Cygni A. McKellar and R. M. Petrie
Discussion
Part VI. Physical Sources Causing Instability:
22. Stars of T. Tauri and UV Ceti types and the phenomenon of continuous emission V. A. Ambartsumian
Addendum to the preceding paper
23. Possible sources of instability in stars P. Ledoux
Discussion.

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