H? LINE IN 36 LYNCIS. II. RETICON OBSERVATIONS OF LINE VARIABILITY

التفاصيل البيبلوغرافية
العنوان:	H? LINE IN 36 LYNCIS. II. RETICON OBSERVATIONS OF LINE VARIABILITY
المؤلفون:	Takada-Hidai, M., Aikman, G. C. L.
المصدر:	Publications of the Astronomical Society of the Pacific; August 1989, Vol. 101 Issue: 642 p699-704, 6p
مستخلص:	High-resolution, high signal-to-noise spectroscopic observations at H-alpha of the helium-weak star 36 Lyncis (HD 79158) confirm the lack of emission and lack of line asymmetry reported earlier, but do reveal line-strength variability on a rapid time scale. This result is discussed in relation to a magnetospheric oblique rotator model recently proposed to explain the known C IV ultraviolet line and magnetic-field variability of the star.
قاعدة البيانات:	Supplemental Index

الوصف
تدمد:	00046280 15383873
DOI:	10.1086/132492