ON THE PECULAR STARFORMING REGION AND DIFFUSE UV-EMISSION IN OMEGA NEBULA

Authors

  • K. G. Dzhakusheva Fesenkov Astrophysical Institute of National Center of Space Researches and Technologies, Almaty, Kazakhstan
  • E. G. Mychelkin Fesenkov Astrophysical Institute of National Center of Space Researches and Technologies, Almaty, Kazakhstan
  • T. B. Simakova Moscow State Industrial University, Moscow, Russia
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Abstract

We continue to proceed with the estimations of peripheral effects of a soft X-ray and possible rigid UV emission to be a result of high activity of other star-forming regions in the nebulae as it has been discussed in 2008 [1,2] for the ORION(M42)-nebula. This year on the base of analysis of the electron density, ionization degree and absorption throughout the OMEGA(M17)-nebula the probable peculiar region of the anomalous diffuse UV emission is proposed as a result of influence of the compact HII regions with a high star-forming activity.

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How to Cite

Dzhakusheva, K. G., Mychelkin, E. G., & Simakova, T. B. (2021). ON THE PECULAR STARFORMING REGION AND DIFFUSE UV-EMISSION IN OMEGA NEBULA. THE JOURNAL OF THE OPEN SYSTEMS EVOLUTION PROBLEMS, 11(1), 28–38. Retrieved from https://peos.kaznu.kz/index.php/peos/article/view/159

Issue

Vol. 11 No. 1 (2009): ЖУРНАЛ ПРОБЛЕМ ЭВОЛЮЦИИ ОТКРЫТЫХ СИСТЕМ

Section

ФИЗИКА