COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 3113 Konkoly Observatory Budapest 27 November 1987 HU ISSN 0374-0676 A REMARK ON TV CYGNI My attention was drawn to this star by the two discordant spectral class data given in the General Catalogues of Variable Stars 1963 and 1985: MO in the main table (source not specified) and GO in the remarks (according to Metik, 1960). A study of literature yielded the following results: 1. The announcement of variability of BD +46 2970 = TV Cyg (Kohl, 1900) is based on a misunderstanding. Kohl compared his visual impression with the chart of Williams (1900), which had been drawn according to the photographic (blue-sensitive) aspect and which naturally shows this reddish star much fainter than it looks visually. 2. A similar error is due to Metik (1960). In his table the wrong identification of star +46d2 of figure 16 (chart 9) with BD+46 2970 is excusable, because on his photographic material the true BD +46 2970 - just visible 1.5 minutes of arc southwest of +46 2 near the edge of the reproduced area - is distinctly fainter than the latter. 3. Conclusion: As supposed also by several photometric observers BD+46 2970= TV Cyg is not variable with high probability. Vyssotsky and Balz (1958) gave the spectral type K2, while Gaposchkin (1939) assigned a spectral type of M to this star. W. WENZEL Sternwarte Sonneberg Zentralinstitut fur Astrophysik der Akademie der Wissenschaften der DDR References: Gaposchkin, S., 1939, Harvard Ann. 108, 6 [BIBCODE 1939AnHar.108....1G ] Kohl, T., 1900, Astron. Nachr. 154, 13 [BIBCODE 1900AN....154...13K ] Metik, L.P., 1960, Izv, Krymskoj Astrofiz. Obs. 23, 60 [BIBCODE 1960IzKry..23...60M ] Vyssotsky, A.N., and Balz, A.G.A., 1958, Publ. Leander McCormick Obs. Virginia 13, II, 118 Williams, A.S., 1900, Astron. Nachr. 152, 77 [BIBCODE 1900AN....152...77W ]