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: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1993 |
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| Umfang: |
7 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Astrophysics and space science - 1968, 204(1993) vom: Feb., Seite 191-197 |
| Übergeordnetes Werk: |
volume:204 ; year:1993 ; month:02 ; pages:191-197 ; extent:7 |
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(DE-627)NLEJ193052784 DE-627 ger DE-627 rakwb eng An o-c diagram analysis of PV cassiopeiae 1993 7 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Krzesiński, J. oth Pajdosz, G. oth Dróżdż, M. oth in Astrophysics and space science 1968 204(1993) vom: Feb., Seite 191-197 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:204 year:1993 month:02 pages:191-197 extent:7 http://dx.doi.org/10.1007/BF00658023 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 204 1993 2 191-197 7 |
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(DE-627)NLEJ193052784 DE-627 ger DE-627 rakwb eng An o-c diagram analysis of PV cassiopeiae 1993 7 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Krzesiński, J. oth Pajdosz, G. oth Dróżdż, M. oth in Astrophysics and space science 1968 204(1993) vom: Feb., Seite 191-197 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:204 year:1993 month:02 pages:191-197 extent:7 http://dx.doi.org/10.1007/BF00658023 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 204 1993 2 191-197 7 |
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(DE-627)NLEJ193052784 DE-627 ger DE-627 rakwb eng An o-c diagram analysis of PV cassiopeiae 1993 7 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Krzesiński, J. oth Pajdosz, G. oth Dróżdż, M. oth in Astrophysics and space science 1968 204(1993) vom: Feb., Seite 191-197 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:204 year:1993 month:02 pages:191-197 extent:7 http://dx.doi.org/10.1007/BF00658023 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 204 1993 2 191-197 7 |
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(DE-627)NLEJ193052784 DE-627 ger DE-627 rakwb eng An o-c diagram analysis of PV cassiopeiae 1993 7 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 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. Springer Online Journal Archives 1860-2002 Krzesiński, J. oth Pajdosz, G. oth Dróżdż, M. oth in Astrophysics and space science 1968 204(1993) vom: Feb., Seite 191-197 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:204 year:1993 month:02 pages:191-197 extent:7 http://dx.doi.org/10.1007/BF00658023 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 204 1993 2 191-197 7 |
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An o-c diagram analysis of PV cassiopeiae |
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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. |
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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. |
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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. |
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