On the Difference Between the Oosterhoff Types i and II Globular Clusters
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| Veröffentlicht in: | Astrophys. J. 168: No. 3, 381-91 (15 Sep 1971) 381-91 (15 Sep 1971), 1971-09, Vol.168, p.381 |
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| Format: | Artikel |
| Sprache: | eng |
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| container_start_page | 381 |
| container_title | Astrophys. J. 168: No. 3, 381-91 (15 Sep 1971) |
| container_volume | 168 |
| creator | Stobie, R. S. |
| description | |
| doi_str_mv | 10.1086/151094 |
| format | Article |
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| fulltext | fulltext |
| identifier | ISSN: 0004-637X |
| ispartof | Astrophys. J. 168: No. 3, 381-91 (15 Sep 1971), 1971-09, Vol.168, p.381 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_crossref_primary_10_1086_151094 |
| source | Alma/SFX Local Collection |
| subjects | CONFIGURATION DISTRIBUTION HELIUM LOSSES MASS METALS N32120 -Physics-Astrophysics-Stars STAR CLUSTERS STAR CLUSTERS/star period-frequency distribution Oosterhoff Types I and II, RR Lyrae variable, (E/T) STAR EVOLUTION STARS STARS/period-frequency distribution of RR Lyrae, in Oosterhoff Types I and II globular clusters, (E/T) |
| title | On the Difference Between the Oosterhoff Types i and II Globular Clusters |
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