Journal article
Laboratory simulations of supernova shockwaves: Formation of a second shock ahead of a radiative shock
- Abstract:
-
Supernovae launch spherical shocks into the circumstellar medium (CSM). These shocks may interact with both the intergalactic magnetic field (IGM) and local mass accumulations (possibly with their own local magnetic fields). The latter interaction may trigger star formation. The shocks have high Mach numbers and may be radiative. We have created similar shocks in the laboratory by focusing laser pulses onto the tip of a solid pin surrounded by ambient gas; ablated material from the pin rapidl...
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- Publisher copy:
- 10.1063/1.2077240
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Authors
Bibliographic Details
- Journal:
- AIP Conference Proceedings
- Volume:
- 784
- Pages:
- 721-729
- Publication date:
- 2005-09-28
- DOI:
- EISSN:
-
1551-7616
- ISSN:
-
0094-243X
- Source identifiers:
-
127457
Item Description
- Language:
- English
- Keywords:
- Pubs id:
-
pubs:127457
- UUID:
-
uuid:6e243e66-9bd8-4cb5-98ed-3c563d4d33d8
- Local pid:
- pubs:127457
- Deposit date:
- 2012-12-19
Terms of use
- Copyright date:
- 2005
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