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von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 91, No. 544 (1979), p. 796-799
...40677610 40677610 ger GBVCP eng HUTCHINGS, J. B. Hα EMISSION IN CYGNUS X-1 1977 Elektronische...
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    von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 88, No. 523 (1976), p. 279-284
    ...40675885 40675885 ger GBVCP eng HUTCHINGS, J. B. IMAGE ISOCON OBSERVATIONS OF EMISSION LINES IN THE...
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      von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 91, No. 541 (1979), p. 361-364
      ... spectrum shows strong emission in all N III lines, and emission in C III, He II, Si IV, He I, and H as well...
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        von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 95, No. 566 (1983), p. 264-267
        ... indicate a near pole-on (i ~ 20° ) orientation. Emission-line variability suggests a concave accretion disk...
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          von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 96, No. 581 (1984), p. 559-562
          ... emission lines. The period is not definitely established but is probably 0.1662 days. No strong phase...
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            von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 91, No. 543 (1979), p. 657-658
            ... Elektronische Ressource Online-Ressource IUE spectroscopy is presented of the radio variable emission-line star...
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              von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 93, No. 554 (1981), p. 486-489
              ... radio flaring period), with a secondary of mass 1.1-1.5 𝕸⊙ . The broad Balmer emission appears to arise...
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                von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 98, No. 599 (1986), p. 104-109
                ... spectroscopic variations. Emission-line variations are found with pulse phase in both systems, with flux...
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                  von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 99, No. 611 (1987), p. 57-61
                  ... critically dependent on the period and are discussed. Emission lines are weak, and show small but unusual...
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                    von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 98, No. 603 (1986), p. 507-510
                    ... states. The emission-line equivalent widths and their orbital phase dependence do not appear to be...
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                      von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 94, No. 557 (1982), p. 107-112
                      ... during our observations. Emission lines are not eclipsed outside of phase 0.041 (at which phase the V...
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                        von HUTCHINGS, J. B. in Publications of the Astronomical Society of the Pacific : electronic edition Vol. 94, No. 559 (1982), p. 541-547
                        ...⊙ and > 1.5 4 . 𝕸⊙ for the stars. Weak He ıı λ4686 emission is detected. No evidence is found for...
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