The orbit of Phi Cygni measured with long-baseline optical interferometry - Component masses and absolute magnitudes
The orbit of the double-lined spectroscopic binary Phi Cygni, the distance to the system, and the masses and absolute magnitudes of its components are presented via measurements with the Mar III Optical Interferometer. On the basis of a reexamination of the spectroscopic data of Rach & Herbig (1...
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| Veröffentlicht in: | The Astronomical journal 1992-12, Vol.104 (6), p.2217-2223 |
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| container_end_page | 2223 |
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| container_issue | 6 |
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| container_title | The Astronomical journal |
| container_volume | 104 |
| creator | Armstrong, J. T. Hummel, C. A. Quirrenbach, A. Buscher, D. F. Mozurkewich, D. Vivekanand, M. Simon, R. S. Denison, C. S. Johnston, K. J. Pan, X.-P. |
| description | The orbit of the double-lined spectroscopic binary Phi Cygni, the distance to the system, and the masses and absolute magnitudes of its components are presented via measurements with the Mar III Optical Interferometer. On the basis of a reexamination of the spectroscopic data of Rach & Herbig (1961), the values and uncertainties are adopted for the period and the projected semimajor axes from the present fit to the spectroscopic data and the values of the remaining elements from the present fit to the Mark III data. The elements of the true orbit are derived, and the masses and absolute magnitudes of the components, and the distance to the system are calculated. |
| doi_str_mv | 10.1086/116396 |
| format | Article |
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T. ; Hummel, C. A. ; Quirrenbach, A. ; Buscher, D. F. ; Mozurkewich, D. ; Vivekanand, M. ; Simon, R. S. ; Denison, C. S. ; Johnston, K. J. ; Pan, X.-P.</creator><creatorcontrib>Armstrong, J. T. ; Hummel, C. A. ; Quirrenbach, A. ; Buscher, D. F. ; Mozurkewich, D. ; Vivekanand, M. ; Simon, R. S. ; Denison, C. S. ; Johnston, K. J. ; Pan, X.-P.</creatorcontrib><description>The orbit of the double-lined spectroscopic binary Phi Cygni, the distance to the system, and the masses and absolute magnitudes of its components are presented via measurements with the Mar III Optical Interferometer. On the basis of a reexamination of the spectroscopic data of Rach & Herbig (1961), the values and uncertainties are adopted for the period and the projected semimajor axes from the present fit to the spectroscopic data and the values of the remaining elements from the present fit to the Mark III data. 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On the basis of a reexamination of the spectroscopic data of Rach & Herbig (1961), the values and uncertainties are adopted for the period and the projected semimajor axes from the present fit to the spectroscopic data and the values of the remaining elements from the present fit to the Mark III data. The elements of the true orbit are derived, and the masses and absolute magnitudes of the components, and the distance to the system are calculated.</description><subject>Astronomy</subject><subject>Binary and multiple stars</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Spectroscopic binaries. 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J.</au><au>Pan, X.-P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The orbit of Phi Cygni measured with long-baseline optical interferometry - Component masses and absolute magnitudes</atitle><jtitle>The Astronomical journal</jtitle><date>1992-12-01</date><risdate>1992</risdate><volume>104</volume><issue>6</issue><spage>2217</spage><epage>2223</epage><pages>2217-2223</pages><issn>0004-6256</issn><eissn>1538-3881</eissn><coden>ANJOAA</coden><abstract>The orbit of the double-lined spectroscopic binary Phi Cygni, the distance to the system, and the masses and absolute magnitudes of its components are presented via measurements with the Mar III Optical Interferometer. On the basis of a reexamination of the spectroscopic data of Rach & Herbig (1961), the values and uncertainties are adopted for the period and the projected semimajor axes from the present fit to the spectroscopic data and the values of the remaining elements from the present fit to the Mark III data. The elements of the true orbit are derived, and the masses and absolute magnitudes of the components, and the distance to the system are calculated.</abstract><cop>Legacy CDMS</cop><pub>University of Chicago Press</pub><doi>10.1086/116396</doi><tpages>7</tpages></addata></record> |
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| ispartof | The Astronomical journal, 1992-12, Vol.104 (6), p.2217-2223 |
| issn | 0004-6256 1538-3881 |
| language | eng |
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| source | NASA Technical Reports Server; Alma/SFX Local Collection; EZB Electronic Journals Library |
| subjects | Astronomy Binary and multiple stars Earth, ocean, space Exact sciences and technology Spectroscopic binaries. Close binaries Stars |
| title | The orbit of Phi Cygni measured with long-baseline optical interferometry - Component masses and absolute magnitudes |
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