Veröffentlichungen zu Akan, M.C. | ||||||||||||||
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Akan, M. C. |
Light curve variations of the eclipsing binary V367 Cygni in: Astrophysics and space science , ISSN 1572-946X, Vol. 135 (1. 1987), p. 157-167 Zugang: zum Volltext ähnliche Vorschläge |
1987 | |||||||||||
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Akan, M. C. |
Further confirmation of the non-eclipsing nature of the RS CVn system V775 Her in: Astrophysics and space science , ISSN 1572-946X, Vol. 169 (1/2. 1990), p. 159-163 Zugang: zum Volltext ähnliche Vorschläge |
1990 | |||||||||||
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Schneider, H., Pavlovski, K., ... |
V367 Cyg as the interacting binary in: Space science reviews , ISSN 1572-9672, Vol. 50 (1/2. 1989), p. 364-364 Zugang: zum Volltext ähnliche Vorschläge |
1989 | |||||||||||
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Tunca, Z., Keskin, V., ... |
The new light curves and period study of AK Herculis in: Astrophysics and space science , ISSN 1572-946X, Vol. 136 (1. 1987), p. 63-76 Zugang: zum Volltext ähnliche Vorschläge |
1987 | |||||||||||
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Tunca, Z., Keskin, V., ... |
Light variations and flares on V471 tauri in: Astrophysics and space science , ISSN 1572-946X, Vol. 204 (2. 1993), p. 297-304 Zugang: zum Volltext ähnliche Vorschläge |
1993 | |||||||||||
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Íbanoğlu, C., Pekünlü, E.R., ... |
Long-Term Photometry of RT Lacertae: 1. Light and Colour Variation in: Astrophysics and space science , ISSN 1572-946X, Vol. 257 (1. 1997), p. 11-21 Zugang: zum Volltext ähnliche Vorschläge |
1997 | |||||||||||
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Íbanoğlu, C., Pekünlü, E.R., ... |
Long–term Photometry of RT Lacertae: 2. Further Evidence fo a Circumstellar Envelope and MAss Accretion in: Astrophysics and space science , ISSN 1572-946X, Vol. 257 (1. 1997), p. 83-94 Zugang: zum Volltext ähnliche Vorschläge |
1997 | |||||||||||
Abstract The light curves, obtained by the authors of the present paper during the period 1978–1992, of the chromospherically active binary system RT Lac were examined. The average (B–V) colour indices were obtained and corrected for the interstellar extinction. Spectroscopic studies indicate... mehr
Copyright: Copyright 1997 Kluwer Academic Publishers mehr
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