COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1596 Konkoly Observatory Budapest 1979 May 2 THE SPECTRUM OF THE SUSPECTED VARIABLE Gl 851.1 (BD+30d4633) Photoelectric data obtained by Krisciunas (1976) had indicated some peculiarities regarding Gliese 851.1. The star, having spectral type dM0e in Gliese's catalog, was suspected to be variable by a few hundredths of a magnitude. Furthermore, the colors [(B-V) = 1.17, (U-B) = 1.12] were rather blue for the assigned spectral type, and with the listed parallax, the star is a full magnitude below the MS in the color-magnitude diagram. At Dr. Krisciunas' suggestion, we obtained a 40 A mm^-1 spectrogram of the red region of Gl 851.1 at Ritter Observatory on 21 August 1978. The star appears unremarkable in the red; there is no trace of Halpha emission, and the spectral type is dM0-1. We note that a recent blue spectral type by Joy and Abt (1974) is simply dM0, thus confirming that no hydrogen emission is visible. The "e" designation in the spectral type in Gliese's catalog then refers to the presence of only Ca II H and K emission. Gl 851.1 is then almost certainly not a BY Draconis variable, as the BY Dra stars of this spectral type all have emission visible at Halpha. Though a few dM stars without Balmer emission are known to flare (e.g., SZ UMa), such objects have very low rates of flare activity, and it seems unlikely that Gl 851.1 could be a flare star. The nature of the variability of Gl 851.1 and its atypical color indices and absolute magnitude remain unclear. BERNARD W. BOPP Ritter Observatory University of Toledo Toledo, OH 43606 U.S.A. References : Joy, A.H. and Abt, H.A. 1974, Astrophys. J. Supp., 28, 1. [BIBCODE 1974ApJS...28....1J ] Krisciunas, K. 1976, J. Am. Assoc. Var. Star Obs., 5, 74. [BIBCODE 1977JAVSO...5...74K ]