Physical Properties of the Binary Star 12 Persei
We have obtained new radial velocities of the double-lined spectroscopic binary star 12 Persei, whose period is 331 d, and which has been resolved in recent years by speckle interferometry. We derive a solution for the orbital elements from the speckle and radial velocity data simultaneously, and fi...
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| Veröffentlicht in: | The Astronomical journal 1998-06, Vol.115 (6), p.2555-2560 |
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| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
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