Optical photometry and ultraviolet spectroscopy of the flare/BY DRA star G1 182 (V 1005 Ori)

Details Optical photometry and ultraviolet spectroscopy of the flare/BY DRA star G1 182 (V 1005 Ori) Optical photometry and ultraviolet spectroscopy of the flare/BY DRA star G1 182 (V 1005 Ori)

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.206..907b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 206, Feb. 15, 1984, p. 907-918.

Astronomy and Astrophysics

Astronomy

22

Chromosphere, Flare Stars, Stellar Flares, Stellar Rotation, Ultraviolet Spectra, Emission Spectra, Light Curve, Stellar Activity, Ubv Spectra, Visual Photometry, X Ray Sources

Scientific paper

G1 182 was previously reported to be a rapidly rotating BY Dra star which flares at an anomalously high rate. The present observations confirm its BY Dra nature but revise the rotation period, such that it is shown to rotate much more slowly. The time-averaged energy output in flares is shown to be normal for a flare star of its spectral type, and its rate of flaring is normal. IUE spectra show chromospheric features whose surface fluxes compare with those of BY Dra itself.

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