Article
Open Access
Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
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K. Černis
Published/Copyright:
February 8, 2017
Received: 2003-6-15
Published Online: 2017-2-8
Published in Print: 2003-9-1
© 2017
Articles in the same Issue
- 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
Keywords for this article
techniques;
photometric;
Vilnius photometric system-stars;
fundamental parameters;
classification ISM;
extinction;
dust clouds ISM;
individual objects;
Barnard 1
Creative Commons
BY-NC-ND 4.0
Articles in the same Issue
- 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
