Artikel
Open Access
Relation between Light Weakening and Equivalent Widths of Circumstellar NaI D-Lines in Stars with R CRB-Type Variability
-
A. E. Rosenbush
und
A. V. Bondar
Veröffentlicht/Copyright:
8. Februar 2017
Received: 2003-4-16
Revised: 2003-5-23
Published Online: 2017-2-8
Published in Print: 2003-9-1
© 2017
Artikel in diesem Heft
- Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
- Overlapping Open Clusters NGC 1750 and NGC 1758 behind the Taurus Dark Clouds. II. CCD Photometry in the Vilnius System
- Spectral Classification of Faint Carbon Stars
- Relation between Light Weakening and Equivalent Widths of Circumstellar NaI D-Lines in Stars with R CRB-Type Variability
- Photoelectric Vilnius Photometry of Stars in the Mega Proper Motion Field KA 10
- Motion of Test Bodies in a Quasi-Newtonian Potential. I. Qualitative Classification of the Motion Trajectories
- Motion of Test Bodies in a Quasi-Newtonian Potential. II. Comparison with Experiments
Schlagwörter für diesen Artikel
stars;
variable weakening;
spectral lines stars;
circumstellar matter;
light individual;
R CrB;
SU Tau;
SV
Creative Commons
BY-NC-ND 4.0
Artikel in diesem Heft
- Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
- Overlapping Open Clusters NGC 1750 and NGC 1758 behind the Taurus Dark Clouds. II. CCD Photometry in the Vilnius System
- Spectral Classification of Faint Carbon Stars
- Relation between Light Weakening and Equivalent Widths of Circumstellar NaI D-Lines in Stars with R CRB-Type Variability
- Photoelectric Vilnius Photometry of Stars in the Mega Proper Motion Field KA 10
- Motion of Test Bodies in a Quasi-Newtonian Potential. I. Qualitative Classification of the Motion Trajectories
- Motion of Test Bodies in a Quasi-Newtonian Potential. II. Comparison with Experiments
