X-ray emission from the W UMa system TZ Bootis
Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region betw...
Ausführliche Beschreibung
Autor*in: |
Geyer, E. H. [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
1983 |
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Schlagwörter: |
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Anmerkung: |
© D. Reidel Publishing Company 1983 |
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Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 97(1983), 2 vom: Dez., Seite 225-227 |
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Übergeordnetes Werk: |
volume:97 ; year:1983 ; number:2 ; month:12 ; pages:225-227 |
Links: |
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DOI / URN: |
10.1007/BF00653484 |
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Katalog-ID: |
OLC2066150894 |
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10.1007/BF00653484 doi (DE-627)OLC2066150894 (DE-He213)BF00653484-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Geyer, E. H. verfasserin aut X-ray emission from the W UMa system TZ Bootis 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1983 Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. Binary System Transition Region Satellite Measurement Proportional Counter Image Proportional Hoffmann, M. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 97(1983), 2 vom: Dez., Seite 225-227 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:97 year:1983 number:2 month:12 pages:225-227 https://doi.org/10.1007/BF00653484 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_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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 97 1983 2 12 225-227 |
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10.1007/BF00653484 doi (DE-627)OLC2066150894 (DE-He213)BF00653484-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Geyer, E. H. verfasserin aut X-ray emission from the W UMa system TZ Bootis 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1983 Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. Binary System Transition Region Satellite Measurement Proportional Counter Image Proportional Hoffmann, M. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 97(1983), 2 vom: Dez., Seite 225-227 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:97 year:1983 number:2 month:12 pages:225-227 https://doi.org/10.1007/BF00653484 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_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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 97 1983 2 12 225-227 |
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10.1007/BF00653484 doi (DE-627)OLC2066150894 (DE-He213)BF00653484-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Geyer, E. H. verfasserin aut X-ray emission from the W UMa system TZ Bootis 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1983 Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. Binary System Transition Region Satellite Measurement Proportional Counter Image Proportional Hoffmann, M. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 97(1983), 2 vom: Dez., Seite 225-227 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:97 year:1983 number:2 month:12 pages:225-227 https://doi.org/10.1007/BF00653484 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_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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 97 1983 2 12 225-227 |
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10.1007/BF00653484 doi (DE-627)OLC2066150894 (DE-He213)BF00653484-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Geyer, E. H. verfasserin aut X-ray emission from the W UMa system TZ Bootis 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1983 Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. Binary System Transition Region Satellite Measurement Proportional Counter Image Proportional Hoffmann, M. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 97(1983), 2 vom: Dez., Seite 225-227 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:97 year:1983 number:2 month:12 pages:225-227 https://doi.org/10.1007/BF00653484 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_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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 97 1983 2 12 225-227 |
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10.1007/BF00653484 doi (DE-627)OLC2066150894 (DE-He213)BF00653484-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Geyer, E. H. verfasserin aut X-ray emission from the W UMa system TZ Bootis 1983 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1983 Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. Binary System Transition Region Satellite Measurement Proportional Counter Image Proportional Hoffmann, M. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 97(1983), 2 vom: Dez., Seite 225-227 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:97 year:1983 number:2 month:12 pages:225-227 https://doi.org/10.1007/BF00653484 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_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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4700 AR 97 1983 2 12 225-227 |
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X-ray emission from the W UMa system TZ Bootis |
abstract |
Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. © D. Reidel Publishing Company 1983 |
abstractGer |
Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. © D. Reidel Publishing Company 1983 |
abstract_unstemmed |
Abstract HEAO-B (Einstein) satellite measurements with the Imaging Proportional Counter revealed the W UMa binary system TZ Bootis as an X-ray source. It is estimated that the luminosity ratioLx/$ L_{v} $of this system is about $ 10^{−3.8} $ indicating that TZ Bootis is in the transition region between A- and W-type W UMa systems. © D. Reidel Publishing Company 1983 |
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title_short |
X-ray emission from the W UMa system TZ Bootis |
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https://doi.org/10.1007/BF00653484 |
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Hoffmann, M. |
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Hoffmann, M. |
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2024-07-04T03:52:24.186Z |
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