The synchronous rotation of IOTA Pegasi

Details The synchronous rotation of IOTA Pegasi The synchronous rotation of IOTA Pegasi

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..537g&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, July 1984, p. 537, 538.

Astronomy and Astrophysics

Astronomy

4

Astrometry, Binary Stars, Stellar Rotation, Orbital Elements, Spectrum Analysis, Synchronism

Scientific paper

Measured rotation rates of the spectroscopic binary stars ι Peg A
(6.5±0.3 km s-1) and B(5±1 km s-1)
are found to be equal to the orbital synchronization values. The
question of whether synchronization has actually occurred is discussed
and the evidence is found to favor the hypothesis.

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