Planetesimals around nearby millisecond pulsars

Details Planetesimals around nearby millisecond pulsars Planetesimals around nearby millisecond pulsars

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...36..317c&link_type=abstract

In: Planets around pulsars; Proceedings of the Conference, California Inst. of Technology, Pasadena, Apr. 30-May 1, 1992 (A93-36

Astronomy and Astrophysics

Astronomy

Extrasolar Planets, Planetary Systems, Protoplanets, Pulsars, Astronomical Models, Planetary Evolution, Radio Emission

Scientific paper

We predict that it is possible to observe line emissions of OH, CN, and
C2 from the planetesimals around some of the nearby millisecond pulsars,
such as PSR1257+12. Observation of these lines will provide an
independent test of either an existing planetary system or one which is
in the process of formation.

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