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A study of the interstellar gas between the sun and the Sagittarius arm
The velocity field of the interstellar gas is examined in the 345-28 deggalactic longitude interval by means of Ca II K lines in high dispersionspectra. The radial velocities of the K lines are compared with 21-cmself-absorption velocities in both dark clouds (Knapp, 1972) and theextended feature mapped by Riegel and Crutcher (1972). Evidence ispresented to show that the extended +7 km/sec feature is more distantthan 500 pc. Two current hypotheses about the structure of the local gasnear the sun, one based upon a ring of expanding matter, the other beinga linear density-wave perturbation, are compared with the observations.The expanding ring model is in better agreement with the observed K-linevelocities.
| Mesures d'étoiles doubles faites aux Observatoires Yerkes et McDonald
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| Takýmyýldýz: | Yilanci |
| Sað Açýklýk: | 17h43m00.53s |
| Yükselim: | +12°15'29.8" |
| Görünürdeki Parlaklýk: | 9.58 |
| özdevim Sað Açýklýk: | -2.6 |
| özdevim Yükselim: | -9.2 |
| B-T magnitude: | 9.815 |
| V-T magnitude: | 9.6 |
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