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恒星物理. 恒星物理. 观察大质量原恒星中外流聚合的开始
C Carrasco-González1, J M Torrelles2, J Cantó3
1Centro de Radioastronomía y Astrofísica UNAM, Apartado Postal 3-72 (Xangari), 58089 Morelia, Michoacán, Mexico. carrasco@crya.unam.mx.
概括
大规模的原星W75N(B) -VLA 2表现出一个结合的电离风,在18年内从紧变长. 这一观察挑战了同otropic外流模型,支持 toroidal 结构内的偶发风喷射.
科学领域:
- * 天体物理学 * 天体物理学
- * 恒星形成 * 恒星形成
- * 无线电天文学
背景情况:
- * 恒星形成的标准模型预测由积聚盘和磁动力学驱动的聚合流出.
- * 之前的观测表明来自大质量原星的同位流出,与理论预测形成鲜明对比.
研究的目的:
- * 研究来自大质量原恒星W75N(B) -VLA 2的电离风的形态和演变.
- * 将观测证据与恒星形成和原恒星外流的理论模型相协调.
主要方法:
- *使用非常大阵列 (VLA) 进行无线电连续观测.
- *分析了18年时间内原星及其相关水蒸气质星的形态变化.
- * 在 toroidal 密度结构中模拟电离风的演变.
主要成果:
- * W75N(B) -VLA 2显示了一个热的,合并的电离风.
- * 源泉在18年内从一个紧的结构演变为一个长长的结构.
- *水蒸汽质光器外从近乎圆形转变为圆形状,表明从同otropic运动转变为协同运动.
结论:
- * 观察到的进化支持偶发的,短暂的电离风模型.
- *风的形态变化随着它通过 toroidal 密度分层传播.
- *这些发现挑战了对大质量原恒星的纯同otropic外流模型.
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