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- W5997415 abstract "Galactic structure in the direction 1/sup II/ approx equal 102 deg , b/ sup II/ approx equal -l deg is studied. Photometric and spectroscopic results, color excesses, and distances for 340 stars of spectral type earlier than A3 are presented. The area can be divided into three parts: a northern part quite dark, a southern part very clear, and a central part of intermediate darkness. The general histogram of distances and the localization of stars earlier than B2 show the local arm and two groups, the one located at a distance of about 2500 pc that might be an interarm. the other located at a distance of about 4200 pc, in the Perseus arm. These results are in good agreement with the distances of exciting stars near S 132 nebula. At this longitude, neutral hydrogen and interstellar calcium lines have two components which correspond to the radial velocities -30 km s/sup -1/ and -50 km s/sup -1/, confirming the existence of these two groups. (auth)" @default.
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- W5997415 date "1973-09-01" @default.
- W5997415 modified "2023-09-27" @default.
- W5997415 title "Galactic structure in the direction of Cepheus" @default.
- W5997415 hasPublicationYear "1973" @default.
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