THE STAR FORMATION CASCADE IN M17 COMPLEX.

Authors

  • K. G. Dzhakusheva Fesenkov Astrophysical Institute (API) of National Center of Space Researches and Technologies, Almaty, RK
  • E. G. Mychelkin Fesenkov Astrophysical Institute (API) of National Center of Space Researches and Technologies, Almaty, RK
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Abstract

We consider the cascade process of star formation in M17 revealed by the world astronomical practice beginning with a pioneer investigation in API of some peculiar active domain of that nebula. The different spectral and IR data including those obtained by space-craft telescopes are discussed in relation with a shock-wave mechanism of production of diffuse X-Rays and (hard) UV [1].

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How to Cite

Dzhakusheva, K. G., & Mychelkin, E. G. (2021). THE STAR FORMATION CASCADE IN M17 COMPLEX. THE JOURNAL OF THE OPEN SYSTEMS EVOLUTION PROBLEMS, 11(2), 13–21. Retrieved from https://peos.kaznu.kz/index.php/peos/article/view/186

Issue

Vol. 11 No. 2 (2009): ЖУРНАЛ ПРОБЛЕМ ЭВОЛЮЦИИ ОТКРЫТЫХ СИСТЕМ

Section

ФИЗИКА