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The infrared massive stellar content of M?83

机译:M?83的红外星体含量

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Aims. We present an analysis of archival Spitzer images and new ground-based and Hubble Space Telescope (HST) near-infrared (IR) and optical images of the field of M?83 with the goal of identifying rare, dusty, evolved massive stars. Methods. We present point source catalogs consisting of 3778 objects from Spitzer Infrared Array Camera (IRAC) Band 1 (3.6 μm) and Band 2 (4.5 μm), and 975 objects identified in Magellan 6.5 m FourStar near-IR J and Ks images. A combined catalog of coordinate matched near- and mid-IR point sources yields 221 objects in the field of M?83. Results. We find 49 strong candidates for massive stars which are very promising objects for spectroscopic follow-up. Based on their location in a B ? V versus V ? I diagram, we expect at least 24, or roughly 50%, to be confirmed as red supergiants.
机译:目的我们对Spitzer影像,新的地面和哈勃太空望远镜(HST)的近红外(IR)以及M?83场的光学影像进行分析,目的是识别稀有,尘土飞扬,演化的大质量恒星。方法。我们提出了点源目录,其中包括来自Spitzer红外阵列摄像机(IRAC)波段1(3.6μm)和波段2(4.5μm)的3778个对象,以及在麦哲伦6.5 m FourStar近红外J和Ks图像中识别出的975个对象。坐标匹配的近红外和中红外点源的组合目录在M?83字段中产生221个对象。结果。我们找到了49个强质量恒星候选者,它们是光谱学后续研究中很有希望的对象。根据它们在B中的位置? V对V?根据我的图表,我们预计至少有24个或大约50%被确认为红色超级巨人。

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