The helium-to-hydrogen ratio of the UV-bright star Barnard 29 of Messier 13

التفاصيل البيبلوغرافية
العنوان: The helium-to-hydrogen ratio of the UV-bright star Barnard 29 of Messier 13
المؤلفون: Adelman, S. J, Aikman, G. C. L, Hayes, D. S, Philip, A. G. D, Sweigart, A. V
المصدر: Astronomy and Astrophysics. 282(1)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 1994.
سنة النشر: 1994
مصطلحات موضوعية: Astronomy
الوصف: Barnard 29 is the most luminous UV-bright star of the globular cluster Messier 13. Comparison of its reddening corrected optical region spectrophotometry and IUE low dispersion fluxes and its H-gamma profile with the predictions of metal-poor model atmospheres having the metallicity of M 13 indicated T(sub eff) = 20250 K, log g = 3.15. Observations of He I lambda(4026) taken with echelle spectrograph of the Multi-Mirror telescope using a Reticon detector show that He/H = 0.055 +/- 0.020. Some astrophysical implications of this result are discussed.
نوع الوثيقة: Report
اللغة: English
تدمد: 0004-6361
URL الوصول: https://ntrs.nasa.gov/citations/19950039092
ملاحظات: RTOP 188-41-51
رقم الانضمام: edsnas.19950039092
قاعدة البيانات: NASA Technical Reports