TU Ophiuchi: Mira variable — Not dwarf nova
Letter to the Editor
Received:
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Abstract
High-speed photometry, spectroscopy, and visual observations of TU Oph show it to be a Mira variable, not a dwarf nova as originally classified or a UV Cet star as tentatively classified.
Keywords
Spectroscopy Visual Observation Dwarf Nova Mira Variable
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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References
- Himpel, K.: 1944,Beob.-Zirk. 26, 25.Google Scholar
- Hoffmeister, C. F.: 1928,Mitt. Sonneberg, No. 13.Google Scholar
- Khopolov, P. N.: 1985,General Catalogue of Variable Stars, Moscow.Google Scholar
- Ledoux, P. and Walraven, Th.: 1958, in S. Flügge (ed.),Handb. der Phys. 51, 410.Google Scholar
- Merrill, P. W., Deutsch, A. J., and Keenan, P. C.: 1962,Astrophys. J. 136, 21.Google Scholar
- Stone, R. P. S. and Baldwin, J. A.: 1983,Monthly Notices Roy. Astron Soc. 204, 347.Google Scholar
- Pickering, E. C.: 1904,Astron. Nachr. 3994, 161.Google Scholar
- Vogt, N. and Bateson, F. M.: 1982,Astron. Astrophys. Suppl. 48, 383.Google Scholar
- Walker, A. D. and Olmsted, M.: 1958,Publ. Astron. Soc. Pacific 70, 495.Google Scholar
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© Kluwer Academic Publishers 1988