An o-c diagram analysis of PV cassiopeiae
Abstract Basing on recent and old photoelectric times of minimum, a new slightly longer period of the apsidal motion for an eclipsing binary PV Cas has been obtained. A difference between observed and theoretical periods of the apsidal motion estimated on the base of Claret and Gimenez models growed...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Krzesiński, J. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1993 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1993 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 204(1993), 2 vom: Juni, Seite 191-197 |
|---|---|
| Übergeordnetes Werk: |
volume:204 ; year:1993 ; number:2 ; month:06 ; pages:191-197 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00658023 |
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OLC2066193453 |
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Abstract Basing on recent and old photoelectric times of minimum, a new slightly longer period of the apsidal motion for an eclipsing binary PV Cas has been obtained. A difference between observed and theoretical periods of the apsidal motion estimated on the base of Claret and Gimenez models growed up to 30 years is found. © Kluwer Academic Publishers 1993 |
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Abstract Basing on recent and old photoelectric times of minimum, a new slightly longer period of the apsidal motion for an eclipsing binary PV Cas has been obtained. A difference between observed and theoretical periods of the apsidal motion estimated on the base of Claret and Gimenez models growed up to 30 years is found. © Kluwer Academic Publishers 1993 |
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Abstract Basing on recent and old photoelectric times of minimum, a new slightly longer period of the apsidal motion for an eclipsing binary PV Cas has been obtained. A difference between observed and theoretical periods of the apsidal motion estimated on the base of Claret and Gimenez models growed up to 30 years is found. © Kluwer Academic Publishers 1993 |
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