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Experimental characterization of the interaction zone between counter propagating Taylor Sedov blast waves

Abstract:

Astronomical observations reveal that the interaction between shock waves and/or blast waves with astrophysical objects (molecular clouds, stars, jets winds etc.) is a common process which leads to a more intricate structure of the Interstellar medium (ISM). In particular, when two isolated massive stars are relatively close and explode, the resulting Supernovae Remnants (SNR) can interact. The impact zone presents fascinating complex hydrodynamic physics which depends on the age of the SNRs,...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1063/1.5137795

Authors


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Name:
Engineering & Physical Sciences Research Council
Grant:
EP/M022331/1
Publisher:
AIP Publishing
Journal:
Physics of Plasmas More from this journal
Volume:
27
Issue:
2
Article number:
022111
Publication date:
2020-02-13
Acceptance date:
2020-01-13
DOI:
EISSN:
1089-7674
ISSN:
1070-664X
Language:
English
Keywords:
Pubs id:
pubs:1082103
UUID:
uuid:ca0b5772-c45f-4d66-b3cb-02fdb16ac233
Local pid:
pubs:1082103
Source identifiers:
1082103
Deposit date:
2020-01-13

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