Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242p..17e&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 1, 1990, p. 17P-19P. Research supported by NS
Astronomy and Astrophysics
Astronomy
7
Eclipsing Binary Stars, Infrared Astronomy, Pulsars, Color-Color Diagram, Light Curve, Stellar Winds
Scientific paper
2.2-micron images have been taken, over the entire range of orbital phase, of the eclipsing millisecond pulsar 1957 + 20. It is shown that the 2.2 micron flux from the pulsar system is variable and that the infrared light curve is similar to the optical light curve. Four additional images at 1.2 micron show that there is a possible infrared excess from the system.
Becklin Eric E.
Eales Stephen A.
McLean Ian S.
Zuckerman Ben
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