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Kopeikin, S. M., Ozernoy, L. M. (1999) Post‐Newtonian Theory for Precision Doppler Measurements of Binary Star Orbits. The Astrophysical Journal, 523 (2). 771-785 doi:10.1086/307759

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Reference TypeJournal (article/letter/editorial)
TitlePost‐Newtonian Theory for Precision Doppler Measurements of Binary Star Orbits
JournalThe Astrophysical Journal
AuthorsKopeikin, S. M.Author
Ozernoy, L. M.Author
Year1999 (October)Volume523
Issue2
PublisherIOP Publishing
DOIdoi:10.1086/307759Search in ResearchGate
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Mindat Ref. ID3347089Long-form Identifiermindat:1:5:3347089:4
GUID0
Full ReferenceKopeikin, S. M., Ozernoy, L. M. (1999) Post‐Newtonian Theory for Precision Doppler Measurements of Binary Star Orbits. The Astrophysical Journal, 523 (2). 771-785 doi:10.1086/307759
Plain TextKopeikin, S. M., Ozernoy, L. M. (1999) Post‐Newtonian Theory for Precision Doppler Measurements of Binary Star Orbits. The Astrophysical Journal, 523 (2). 771-785 doi:10.1086/307759
In(1999, October) The Astrophysical Journal Vol. 523 (2) IOP Publishing

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Jaroszyński, M. (1999) Prospects for the Determination of Star Orbits near the Galactic Center. The Astrophysical Journal, 521 (2). 591-596 doi:10.1086/307588
Kopeikin, S. M. (1994) Supplementary parameters in the parameterized post-Keplerian formalism. The Astrophysical Journal, 434. doi:10.1086/187576
Haugan, M. P. (1985) Post-Newtonian arrival-time analysis for a pulsar in a binary system. The Astrophysical Journal, 296. 1pp. doi:10.1086/163414
Kopeikin, S. M. (1996) Proper Motion of Binary Pulsars as a Source of Secular Variations of Orbital Parameters. The Astrophysical Journal, 467 (2). doi:10.1086/310201
Portilla, M., Lapiedra, R. (1984) Long-term post-Newtonian effects in a binary system. The Astrophysical Journal, 286. 633pp. doi:10.1086/162638
McGaugh, Stacy S. (1999) Distinguishing between Cold Dark Matter and Modified Newtonian Dynamics: Predictions for the Microwave Background. The Astrophysical Journal, 523 (2). doi:10.1086/312274
Calder, Alan C., Wang, Edward Y. M. (2002) Numerical Models of Binary Neutron Star System Mergers. II. Coalescing Models with Post‐Newtonian Radiation Reaction Forces. The Astrophysical Journal, 570 (1). 303-313 doi:10.1086/339743
Hiscock, W. A., Lindblom, L. (1979) Post-Newtonian effects on satellite orbits near Jupiter and Saturn. The Astrophysical Journal, 231. 224pp. doi:10.1086/157184
Klioner, S. A., Kopeikin, S. M. (1994) The post-Keplerian orbital representations of the relativistic two-body problem. The Astrophysical Journal, 427. 951pp. doi:10.1086/174201
Seymour, Diana M., Mason, Brian D., Hartkopf, William I., Wycoff, Gary L. (2002) Binary Star Orbits. II. Preliminary First Orbits for 117 Systems. The Astronomical Journal, 123 (2). 1023-1038 doi:10.1086/338441
Lee, D. L., Ni, W.-T., Caves, C. M., Will, C. M. (1976) Theoretical frameworks for testing relativistic gravity. V - Post-Newtonian limit of Rosen's theory. The Astrophysical Journal, 206. 555pp. doi:10.1086/154412
 
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