Wolf-Rayet stars and relativistic objects

A M Cherepashchuk

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Wolf-Rayet stars and relativistic objects

机译：Wolf-Rayet星和相对论天体

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Wolf-Rayet (WR) stars, identified by strong broad mission lines of helium, nitrogen, carbon, and oxygen at different ionization states, were discovered by French astronomers M Wolf and G Rayet in 1867 [1]. We shall consider only massive (m = 5-50M_⊙) WR stars of the galactic type I population, which concentrate on average towards the galactic plane. Low-mass hot stars observed as nuclei of planetary nebulae also exhibit WR signatures; we shall not consider them in the present paper.

机译：Wolf-Rayet（WR）恒星是由天文学家M Wolf和G Rayet于1867年发现的，在不同电离状态下氦，氮，碳和氧具有很强的广泛任务线[1]。我们将仅考虑I型银河种群的大型（m =5-50M_⊙）WR恒星，这些恒星平均集中在银河平面上。被观测为行星状星云核的低质量热星也显示出WR特征。我们将不在本文中考虑它们。

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《Physics - Uspekhi》 |2002年第8期|共5页
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A M Cherepashchuk;
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正文语种 eng
中图分类物理学;
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1. Wolf-Rayet stars and relativistic objects [J] . A M Cherepashchuk Physics - Uspekhi . 2002,第8期

机译：Wolf-Rayet星和相对论天体
2. Laser Action in the Stellar Atmospheres of Wolf-Rayet Stars and Quasi-Stellar Objects (QSOs) [J] . Millette P. A. Progress in Physics . 2021,第1期

机译：Wolf-rayet恒星和准恒星物体（QSOS）的恒星气氛中的激光动作
3. New code for equilibriums and quasiequilibrium initial data of compact objects. IV. Rotating relativistic stars with mixed poloidal and toroidal magnetic fields [J] . Physical review, D . 2019,第12aPta1期

机译：均衡和QuasiequiBirium初始数据的新代码。 IV。用混合粒子和环形磁场旋转相对论恒星
4. A Post-Newtonian Treatment of Relativistic Compact Object Binaries in Star Clusters [C] . J. M. B. Downing, R. Spurzem International Astronomical Union . 2008

机译：纽托尼亚术后恒星集群中相对论紧凑型对象二进制文件
5. Comparison of clusters with and without detectable Wolf-Rayet stars in starburst galaxies using optical, near-infrared imagery and spectroscopy. [D] . Buckalew, Brent Alan. 2003

机译：使用光学，近红外图像和光谱学比较星爆星系中有和没有可检测到的沃尔夫-瑞叶星的星团。
6. Nova Geminorum No. 2 as a Wolf-Rayet Star [O] . Walter S. Adams, Francis G. Pease 1915

机译：诺瓦·杰米诺鲁姆2号作为沃尔夫·瑞叶星
7. Continuum and emission line observations of Wolf-Rayet stars: single and “WR+abs” objects [O] . Patrick W. Morris 1995

机译：Wolf-Rayet Stars的连续统一和排放线观察：单身和“WR + ABS”对象
8. Clue to the Extent of Convective Mixing Inside Massive Stars: The Surface Hydrogen Abundances of Luminous Blue Variables and Hydrogen-Poor Wolf-Rayet Stars [R] . Stothers, R. B. , Chin, C. 1999

机译：大质量恒星内部对流混合程度的线索：发光蓝变量和贫氢狼群的恒星表面氢丰度

Wolf-Rayet stars and relativistic objects

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