Orbital elements of PSR B1620-26

Details Orbital elements of PSR B1620-26 Orbital elements of PSR B1620-26

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...432..239m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 432, no. 1, p. 239-241

Astronomy and Astrophysics

Astrophysics

11

Astronomical Models, Binary Stars, Celestial Mechanics, Mathematical Models, Orbit Calculation, Orbital Elements, Orbital Mechanics, Pulsars, Three Body Problem, Triple Stars, Eccentric Orbits, Equations Of Motion, Periodic Variations, Stellar Orbits, Trajectory Analysis

Scientific paper

We show that the third body around the binary pulsar B1620-26 can have
virtually any mass. We also show that observations over the next decade
should largely solve for the orbital elements of the system (with the
usual exception of the inclination).

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