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The binary progenitor of Tycho Brahe's 1572 supernova

The binary progenitor of Tycho Brahe's 1572 supernova

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_743496765

The binary progenitor of Tycho Brahe's 1572 supernova

About this item

Full title

The binary progenitor of Tycho Brahe's 1572 supernova

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2004-10, Vol.431 (7012), p.1069-1072

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

The brightness of type Ia supernovae, and their homogeneity as a class, makes them powerful tools in cosmology, yet little is known about the progenitor systems of these explosions. They are thought to arise when a white dwarf accretes matter from a companion star, is compressed and undergoes a thermonuclear explosion
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Alternative Titles

Full title

The binary progenitor of Tycho Brahe's 1572 supernova

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_743496765

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_743496765

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/nature03006

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