Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri
Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Caracatsanis, V. A. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1977 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1977 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 47(1977), 2 vom: Apr., Seite 375-384 |
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| Übergeordnetes Werk: |
volume:47 ; year:1977 ; number:2 ; month:04 ; pages:375-384 |
| Links: |
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| DOI / URN: |
10.1007/BF00642845 |
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OLC2066129739 |
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| 520 | |a Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. | ||
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10.1007/BF00642845 doi (DE-627)OLC2066129739 (DE-He213)BF00642845-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Caracatsanis, V. A. verfasserin aut Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. Frequency Domain Domain Analysis Light Curf Frequency Domain Analysis Light Change Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 47(1977), 2 vom: Apr., Seite 375-384 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:47 year:1977 number:2 month:04 pages:375-384 https://doi.org/10.1007/BF00642845 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 47 1977 2 04 375-384 |
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10.1007/BF00642845 doi (DE-627)OLC2066129739 (DE-He213)BF00642845-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Caracatsanis, V. A. verfasserin aut Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. Frequency Domain Domain Analysis Light Curf Frequency Domain Analysis Light Change Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 47(1977), 2 vom: Apr., Seite 375-384 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:47 year:1977 number:2 month:04 pages:375-384 https://doi.org/10.1007/BF00642845 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 47 1977 2 04 375-384 |
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10.1007/BF00642845 doi (DE-627)OLC2066129739 (DE-He213)BF00642845-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Caracatsanis, V. A. verfasserin aut Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. Frequency Domain Domain Analysis Light Curf Frequency Domain Analysis Light Change Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 47(1977), 2 vom: Apr., Seite 375-384 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:47 year:1977 number:2 month:04 pages:375-384 https://doi.org/10.1007/BF00642845 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 47 1977 2 04 375-384 |
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10.1007/BF00642845 doi (DE-627)OLC2066129739 (DE-He213)BF00642845-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Caracatsanis, V. A. verfasserin aut Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. Frequency Domain Domain Analysis Light Curf Frequency Domain Analysis Light Change Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 47(1977), 2 vom: Apr., Seite 375-384 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:47 year:1977 number:2 month:04 pages:375-384 https://doi.org/10.1007/BF00642845 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 47 1977 2 04 375-384 |
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10.1007/BF00642845 doi (DE-627)OLC2066129739 (DE-He213)BF00642845-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Caracatsanis, V. A. verfasserin aut Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri 1977 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1977 Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. Frequency Domain Domain Analysis Light Curf Frequency Domain Analysis Light Change Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 47(1977), 2 vom: Apr., Seite 375-384 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:47 year:1977 number:2 month:04 pages:375-384 https://doi.org/10.1007/BF00642845 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 47 1977 2 04 375-384 |
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Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri |
| abstract |
Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. © D. Reidel Publishing Company 1977 |
| abstractGer |
Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. © D. Reidel Publishing Company 1977 |
| abstract_unstemmed |
Abstract The aim of this paper has been to carry out an analysis of the light curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method of the analysis of the light curves of eclipsing systems in the frequency domain. The elements of these systems are evaluated and the results are discussed. © D. Reidel Publishing Company 1977 |
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2 |
| title_short |
Frequency domain analysis of the light changes of the close eclipsing systems TX ursae majoris and S cancri |
| url |
https://doi.org/10.1007/BF00642845 |
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10.1007/BF00642845 |
| up_date |
2024-07-04T03:49:49.497Z |
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