Rotational modulation and flares on RS Canum Venaticorum and BY Draconis-type stars. XIV - Phase, eclipse and flare observations of YY Geminorum by Exosat and IUE

التفاصيل البيبلوغرافية
العنوان: Rotational modulation and flares on RS Canum Venaticorum and BY Draconis-type stars. XIV - Phase, eclipse and flare observations of YY Geminorum by Exosat and IUE
المؤلفون: Haisch, B. M, Schmitt, J. H. M. M, Rodono, M, Gibson, D. M
المصدر: Astronomy and Astrophysics. 230(2 Ap)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 1990.
سنة النشر: 1990
مصطلحات موضوعية: Astrophysics
الوصف: The eclipsing spectroscopic binary YY Geminorum has been observed at optical, ultraviolet, and X-ray wavelengths for rotational modulation, eclipse variability, and flaring. The epoch T(phi = 0) = JD 2425698.3561, and the phase P = 0.81428224 d. The quiescent level of Mg II emission is remarkably steady during the three-year observing interval, with F(Mg II) roughly 3.6 x 10 to the -12th erg/sq cm/s. Both stars appear to have identical Mg II surface fluxes, with F roughly 1.8 x 10 to the 6th erg/sq cm/s. Both stars appear to be covered with evenly distributed Mg II emitting regions consistent with the proposition of Doyle (1987) that saturation of the Mg II lines occurs for stars having P less than 4 d, implying that such stars are entirely covered by plage. The transition region lines show significantly more rotational modulation and/or secular variability than Mg II. Both Mg II and the transition region lines show preflare and postflare enhancement.
نوع الوثيقة: Report
اللغة: English
تدمد: 0004-6361
URL الوصول: https://ntrs.nasa.gov/citations/19900062532
ملاحظات: NASA ORDER H-85057-B

NAS5-28720
رقم الأكسشن: edsnas.19900062532
قاعدة البيانات: NASA Technical Reports