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HIGH MASS STAR FORMATION IN THE MOLECULAR CLOUD COMPLEX NGC 6334: NGC 6334E

机译:分子云复杂NGC 6334中的高质量恒星形成:NGC 6334E

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摘要

We obtained deep broad-band JHK_s and narrowband H_2 and Brγ images of the northern part of the giant molecular cloud NGC 6334 containing three distinct centers of star formation (NGC 6334IN, E, and F), probably at different evolutionary stages. Preliminary results, including mid-IR images at 9.8 and 11.9 μm of the shell-shaped HII region NGC 6334E, are presented. An embedded young stellar cluster composed mainly by intermediate-mass stars (earlier than B3-B4) and by low-mass stars has been found within the boundaries of the HII region. At the center of the region we detected a Class Ⅰ young stellar object with an infrared luminosity of ~ 8 solar luminosity.
机译:我们获得了巨型分子云NGC 6334北部的深宽带JHK_s和窄带H_2和Brγ图像,其中包含三个不同的恒星形成中心(NGC 6334IN,E和F),可能处于不同的演化阶段。初步结果包括壳形HII区域NGC 6334E的9.8和11.9μm的中红外图像。在HII区域的边界内发现了一个嵌入的年轻恒星群,主要由中等质量的恒星(比B3-B4早)和低质量的恒星组成。在该区域的中心,我们发现了一个Ⅰ类年轻的恒星物体,其红外光度为〜8太阳光度。

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