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- W2023863601 abstract "view Abstract Citations (43) References (19) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Evidence for a Planet around the Pulsar PSR B0329+54 Shabanova, Tatiana V. Abstract The data set of available pulse arrival times of the pulsar PSR B0329+54, including the JPL timing data between 1968 and 1983 and the Pushchino timing data between 1978 and 1994, is analyzed. It is shown that a quasi-sinusoidal modulation with a period of 16.9 yr exists in the timing residuals. This periodicity can be interpreted as evidence for the existence of a planet-like body orbiting the pulsar PSR B0329+54 with a 16.9 yr orbital period. The planet has a minimum mass of about twice the mass of Earth and moves in eccentric orbit (e = 0.23) with a semimajor axis of 7.3 AU. The existence of 3 yr periodicity in arrival times, claimed by Demianski & Proszynski in 1979, is verified. It manifested itself distinctly in the JPL data only after removing the main 16.9 yr periodicity. Publication: The Astrophysical Journal Pub Date: November 1995 DOI: 10.1086/176440 Bibcode: 1995ApJ...453..779S Keywords: STARS: PLANETARY SYSTEMS; STARS: PULSARS: INDIVIDUAL ALPHANUMERIC: PSR B0329+54 full text sources ADS | data products SIMBAD (2)" @default.
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- W2023863601 date "1995-11-01" @default.
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- W2023863601 title "Evidence for a Planet around the Pulsar PSR B0329+54" @default.
- W2023863601 doi "https://doi.org/10.1086/176440" @default.
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