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在猎户座的一个巨大的原星的反射红外光谱
J I Morino1, T Yamashita, T Hasegawa
1Institute of Astronomy, The University of Tokyo, Osawa, Mitaka, Japan. morino@mtk.ioa.s.u-tokyo.ac.jp
Nature
|June 10, 1998
概括
在Orion-KL中,巨大的年轻恒星被尘埃遮蔽. 反射的红外光显示出一个惊人的大半径和高积累率,挑战目前的恒星形成理论.
科学领域:
- 天文学 天文学
- 天体物理学 天体物理学
- 星星形成 星星形成
背景情况:
- 猎户座-KL中的红外源IRc2是一个巨大的,年轻的恒星,被一个密集的,盘状的外遮蔽.
- 由于可见度有限,它的确切性质和进化阶段尚不清楚.
研究的目的:
- 为了研究隐蔽的红外源IRc2.2的特性.
- 为了确定大质量年轻恒星的积聚率和物理特征.
主要方法:
- 对反射的红外辐射的观测 (大约. 2微米) 在极地方向逃逸.
- 对反射光谱的分析,包括金属原子和一氧化碳的吸收线.
主要成果:
- 反射的光谱显示源温度大约为4500K.
- 源的亮度意味着半径至少为300个太阳半径.
- 所需的积累率估计为每年 (5-15) × 10(-3) 太阳质量.
结论:
- 推断的半径太大了,对于目前的大质量恒星形成模型而言,其增积率适度.
- 积累速率必须比通常假设的要高得多 (至少要大两倍).
- 这些发现挑战了关于大质量恒星形成的现有理论.
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