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X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC

X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2092755030

X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC

About this item

Full title

X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2018-08

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

The Large Magellanic Cloud (LMC) has \(\sim\)60 confirmed supernova remnants (SNRs). Because of the known distance, 50 kpc, the SNRs' angular sizes can be converted to linear sizes, and their X-ray observations can be used to assess X-ray luminosities (\(L_X\)). We have critically examined the LMC SNRs' sizes reported in the literature to determine...

Alternative Titles

Full title

X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2092755030

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2092755030

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1808.01435

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