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Kelvin–Helmholtz instabilities as the source of inhomogeneous mixing in nova explosions

Kelvin–Helmholtz instabilities as the source of inhomogeneous mixing in nova explosions

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_901000794

Kelvin–Helmholtz instabilities as the source of inhomogeneous mixing in nova explosions

About this item

Full title

Kelvin–Helmholtz instabilities as the source of inhomogeneous mixing in nova explosions

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2011-10, Vol.478 (7370), p.490-492

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

The isotope mix from classic supernovae
The chemical abundance pattern of the Universe is largely dependent on the products of the nucleosynthesis that occurs during stellar explosions. Classical novae are thought to be the main sources of
15
N,
17
O and
13
C isotopes in our Galaxy, but the origin of the inhomogeneous distribut...

Alternative Titles

Full title

Kelvin–Helmholtz instabilities as the source of inhomogeneous mixing in nova explosions

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_901000794

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_901000794

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/nature10520

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