The period of the intermediate polar AO PSC (= H2252-035)

Details The period of the intermediate polar AO PSC (= H2252-035) The period of the intermediate polar AO PSC (= H2252-035)

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207p..17w&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, March 15, 1984, p. 17P-21P.

Astronomy and Astrophysics

Astronomy

7

Binary Stars, Orbital Elements, Stellar Mass Accretion, Stellar Spectrophotometry, Maxima, Neutron Stars, Stellar Rotation

Scientific paper

Photometry of the intermediate polar AO Psc (=H2252-035) is reported. An
upper limit of less than 8.5 x 10 to the -7th/yr is derived for the rate
of change of the spin period of the accreting object, thus ruling out a
neutron star. The importance of future monitoring of these systems is
emphasized.

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