Three classical Cepheid variable stars in the nuclear bulge of the Milky Way
Three classical Cepheid variable stars in the nuclear bulge of the Milky Way
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Author / Creator
Matsunaga, N , Kawadu, T , Nishiyama, S , Nagayama, T , Kobayashi, N , Tamura, M , Bono, G , Feast, M W and Nagata, T
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
The nuclear bulge is a region with a radius of about 200 parsecs around the centre of the Milky Way. It contains stars with ages ranging from a few million years to over a billion years, yet its star-formation history and the triggering process for star formation remain to be resolved. Recently, episodic star formation, powered by changes in the ga...
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Full title
Three classical Cepheid variable stars in the nuclear bulge of the Milky Way
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Author / Creator
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Record Identifier
TN_cdi_proquest_journals_2087005042
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2087005042
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1111.6359
