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| dc.contributor.author | Suleimanov, Valery F. | |
| dc.contributor.author | Werner, Klaus | |
| dc.date.accessioned | 2021-01-18T08:22:40Z | |
| dc.date.available | 2021-01-18T08:22:40Z | |
| dc.date.issued | 2020 | |
| dc.identifier.issn | 1432-0746 | |
| dc.identifier.uri | http://hdl.handle.net/10900/111603 | |
| dc.language.iso | en | de_DE |
| dc.publisher | Edp Sciences S A | de_DE |
| dc.relation.uri | http://dx.doi.org/10.1051/0004-6361/202037502 | de_DE |
| dc.subject.ddc | 520 | de_DE |
| dc.subject.ddc | 530 | de_DE |
| dc.title | Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination | de_DE |
| dc.type | Article | de_DE |
| utue.quellen.id | 20200929220116_00661 | |
| utue.personen.roh | Suleimanov, Valery F. | |
| utue.personen.roh | Poutanen, Juri | |
| utue.personen.roh | Werner, Klaus | |
| dcterms.isPartOf.ZSTitelID | Astronomy & Astrophysics | de_DE |
| dcterms.isPartOf.ZS-Issue | A33 | de_DE |
| dcterms.isPartOf.ZS-Volume | 639 | de_DE |
| utue.fakultaet | 07 Mathematisch-Naturwissenschaftliche Fakultät | de_DE |
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