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- W2082897363 abstract "We present photometric observations of four stars that are optical counterparts of soft X-ray/EUV sources, namely 1ES 0829+15.9, 1ES0920-13.6, 2RE J1 10159+223509 and 1ES 1737+61.2. We have discovered periodic variability in two of the stars, viz., MCC 527 (1ES 0829+15.9; Period = 0 d .828 ± 0.0047) and HD 81032 (1ES 0920-13.6; Period = ∼ 57.02 ± 0.560 days). HD 95559 (2RE J1 10159+223509) is found to show a period of 3 d . HD 160934 (1ES1737+61.2) also shows photometric variability but needs to be monitored further for finding its period. These stars most likely belong to the class of chromospherically active stars." @default.
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- W2082897363 date "2002-03-01" @default.
- W2082897363 modified "2023-10-14" @default.
- W2082897363 title "Photometric variability of four coronally active stars" @default.
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- W2082897363 doi "https://doi.org/10.1007/bf02702457" @default.
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