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New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connecti...

New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connecti...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2081321488

New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connection between RCBs, DYPers and ordinary carbon stars

About this item

Full title

New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connection between RCBs, DYPers and ordinary carbon stars

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2009-05

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

R Coronae Borealis stars (RCB) are a rare type of evolved carbon-rich supergiant stars that are increasingly thought to result from the merger of two white dwarfs, called the Double degenerate scenario. This scenario is also studied as a source, at higher mass, of type Ia Supernovae (SnIa) explosions. Therefore a better understanding of RCBs compos...

Alternative Titles

Full title

New Magellanic Cloud R Coronae Borealis and DY Per type stars from the EROS-2 database: the connection between RCBs, DYPers and ordinary carbon stars

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2081321488

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2081321488

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.0905.3224

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