First Mapping Observations of Two Possible Cloud Collision Candidates IRAS 02459+6029 and 05363+3127

Bei Xin, Jun-jie Wang
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引用次数: 3

Abstract

The first mapping observations of the cold infrared sources IRAS 02459+6029 and 05363+3127 in the molecular lines 12CO(1–0), 13CO(1–0) and C18O(1–0) were made using the 13.7 m millimeter wave telescope in Qinghai. Both the integrated intensity maps and position-velocity diagrams show that each has two components adjacent in both space and velocity which means possible cloud-cloud collisions in the two regions. The near-infrared color-color diagram from the 2MASS database reveals that the density of YSOs in the colliding site is much higher than in the surrounding regions. The results appear to indicate that star forming activities have taken place in the two regions due to the cloud-cloud collision. We conclude that both sources are cloud collision candidates.
两个可能的云碰撞候选者IRAS 02459+6029和05363+3127的首次测绘观测
利用青海13.7 m毫米波望远镜对冷红外源IRAS 02459+6029和05363+3127在12CO(1-0)、13CO(1-0)和C18O(1-0)分子谱线进行了首次作图观测。综合强度图和位置-速度图都表明,每个区域都有两个空间和速度相邻的分量,这意味着两个区域可能发生云-云碰撞。来自2MASS数据库的近红外彩色图显示,碰撞现场的yso密度远高于周围区域。结果似乎表明,由于云-云碰撞,这两个区域已经发生了恒星形成活动。我们得出结论,这两个源都是云碰撞候选者。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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