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First UV observations of the optical counterpart of the X-ray source 2S0114+650
Authors:Luciana Bianchi
Institution:(1) ESTEC- Astronomy Division of the European Space Agency, Spain
Abstract:The X-Ray Source 2S0114+650 discovered by SAS-3 in 1978 has been associated with a highly reddened star showing broad Hagr emission.We observed this star with the LWR spectrograph on board the I.U.E. Satellite on Sep. 1980 and Feb. 1981. An Ultraviolet flux was detected longward of the 2200 Å bump, consistent with the B0.5 spectral classification and the values of V=11 and E(B-V)=1.48, The UV extinction in the region around 2200Å seems to deviate from the standard interstellar extinction law.European Space Agency Satellite Tracking Station P.O.Box 54065 — Madrid — SpainBased on observations by the International Ultraviolet Explorer, collected at the Villafranca Satellite Tracking Station of the European Space Agency.
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