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Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant Hi...

Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant Hi...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_1954958273

Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries

About this item

Full title

Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries

Publisher

Dordrecht: Springer Netherlands

Journal title

Space science reviews, 2017-10, Vol.212 (1-2), p.59-150

Language

English

Formats

Publication information

Publisher

Dordrecht: Springer Netherlands

More information

Scope and Contents

Contents

Massive stars, at least

10
times more massive than the Sun, have two key properties that make them the main drivers of evolution of star clusters, galaxies, and the Universe as a whole. On the one hand, the outer layers of massive stars are so hot that they produce most of the ionizing ultraviolet radiation of galaxies; in fact, the firs...

Alternative Titles

Full title

Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_1954958273

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_1954958273

Other Identifiers

ISSN

0038-6308

E-ISSN

1572-9672

DOI

10.1007/s11214-017-0340-1

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