The results of the deepest objective prism low dispersion near-infrared (IV-N+RG695, I=15m.5) spectral survey of the Milky Way (|b| < 5°.2, 50° < l < 115°) are presented. The surface density of Carbon stars reaches its maximum values in the directions of Carina (l=292°.5) and Cygnus-Casiopeae (l=97°.5), which are equal to 2.7 and 2.3 star per sq. deg., respectively. The latitude distribution (|b| < 5°.0) of Carbon stars is uniform.
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机译：近红外线（IV-N + RG695，I = 15M.5）的最佳客观棱镜低分散的结果（| b | <5°.2,50°<115°）的光谱测量提出了。碳恒星的表面密度在Carina（L = 292°0°5）和Cygnus-casiopeae（L = 97°5）的方向上达到其最大值，其每平方米等于2.7和2.3星。Deg。，分别。碳恒星的纬度分布（| b | <5°0）是均匀的。
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