Abstract
Results of the high dispersion spectroscopic observations on HBV 475, V1016 Cyg, and HM Sge are presented. Due to yearly observations of HBV 475 since 1981, radial velocities which have been measured from Hα and Hγ can be explained by a bipolar like non-spherical flow combined with the rotation. Highly resolved profiles of Hα, [FeVII]λ6087, [OIII] λλ4959,5007, and HeIIλ4686 are obtained from V1016 Cyg and HM Sge as well as HBV 475. Characteristic differences of them can be seen among these symbiotic stars.
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Iijima,T., Mammano,A., and Margoni,R. 1981, Ap. and Space Sci. ,75, 237
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© 1988 Kluwer Academic Publishers
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Tamura, S. (1988). Emission Line Analyses of HBV 475, V1016 Cyg, and HM Sge. In: Mikolajewska, J., Friedjung, M., Kenyon, S.J., Viotti, R. (eds) The Symbiotic Phenomenon. Astrophysics and Space Science Library, vol 145. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2969-2_58
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DOI: https://doi.org/10.1007/978-94-009-2969-2_58
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7833-7
Online ISBN: 978-94-009-2969-2
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