The influence of variations of the elemental composition on the thermal properties of gas behind shock fronts
- Authors: Vasiliev E.O.1,2, Shchekinov Y.A.3
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Affiliations:
- Southern Federal University
- Special Astrophysical Observatory
- Astro Space Center, Lebedev Physical Institute
- Issue: Vol 61, No 4 (2017)
- Pages: 342-346
- Section: Article
- URL: https://journals.rcsi.science/1063-7729/article/view/190597
- DOI: https://doi.org/10.1134/S1063772917040175
- ID: 190597
Cite item
Abstract
The homogenization of inhomogeneities in the elemental composition of the interstellar medium due to stellar evolution and weak mixing are inevitably related to the action of shocks. This paper considers the influence of variations in the elemental composition on the thermal and ionizational evolution of a collisional gas with the solar metallicity that is cooled behind a shock front with a velocity of 50–120 km/s. The intensities of lines of heavy elements in plasma cooling behind a shock front depend not only on variations in the elemental composition, but also on the shock velocity, due to the different values of the critical density for the transition to the equilibrium level populations in atoms and ions of heavy elements. This circumstance can be used to determine the elemental composition of cool and warm gas of the interstellar medium, as well as the thermal history of the gas.
About the authors
E. O. Vasiliev
Southern Federal University; Special Astrophysical Observatory
Author for correspondence.
Email: eugstar@mail.ru
Russian Federation, Rostov-on-Don; Karachaevo-Cherkesskaya Republic, 357169
Yu. A. Shchekinov
Astro Space Center, Lebedev Physical Institute
Author for correspondence.
Email: yus@asc.rssi.ru
Russian Federation, Profsoyuznaya ul. 84/32, Moscow, 117997
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