首页> 外文OA文献 >Lithium and magnetic fields in giants. HD 232862 : a magnetic and lithium-rich giant star
【2h】

Lithium and magnetic fields in giants. HD 232862 : a magnetic and lithium-rich giant star

机译:巨人的锂和磁场。 HD 232862:磁性和   富锂巨星

摘要

We report the detection of an unusually high lithium content in HD 232862, afield giant classified as a G8II star, and hosting a magnetic field. With thespectropolarimeters ESPaDOnS at CFHT and NARVAL at TBL, we have collected highresolution and high signal-to-noise spectra of three giants : HD 232862, KU Pegand HD 21018. From spectral synthesis we have inferred stellar parameters andmeasured lithium abundances that we have compared to predictions fromevolutionary models. We have also analysed Stokes V signatures, looking for amagnetic field on these giants. HD 232862, presents a very high abundance oflithium (ALi = 2.45 +/- 0.25 dex), far in excess of the theoretically valueexpected at this spectral type and for this luminosity class (i.e, G8II). Theevolutionary stage of HD 232862 has been precised, and it suggests a mass inthe lower part of the [1.0 Msun ; 3.5 Msun ] mass interval, likely 1.5 to 2.0solar mass, at the bottom of the Red Giant Branch. Besides, a time variableStokes V signature has been detected in the data of HD 232862 and KU Peg,pointing to the presence of a magnetic field at the surface of these tworapidly rotating active stars.
机译:我们报告检测到HD 232862中异常高的锂含量,HD 232862是归类为G8II恒星的巨人,并具有磁场。使用CFHT的旋光仪ESPaDOnS和TBL的NARVAL光谱仪,我们收集了HD 232862,KU Pegand HD 21018这三大巨头的高分辨率和高信噪比光谱。通过光谱合成,我们推导出了恒星参数和与之相比测得的锂丰度进化模型的预测。我们还分析了Stokes V签名,以寻找这些巨星上的无磁场。 HD 232862呈现出非常高的锂含量(ALi = 2.45 +/- 0.25 dex),远远超过了该光谱类型和该亮度等级(即G8II)的理论值。 HD 232862的发展阶段已经过精确调整,它表明在[1.0 Msun;在红巨星分支的底部,质量间隔为3.5 Msun [],可能为1.5至2.0太阳质量。此外,在HD 232862和KU Peg的数据中还检测到了时间变量Stokes V信号,这表明在这两个快速旋转的活动恒星的表面存在磁场。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号