M. Beech et al., ON THE NON-OBSERVABILITY OF METEORS FROM COMET-C 1995-01-HALE-BOPP/, Monthly Notices of the Royal Astronomical Society, 283(1), 1996, pp. 137-140
The possibility of observing enhanced meteoric activity, at Earth, fro
m dust associated with C/1995 01 Hale-Bopp is investigated. We conside
r the nodal distribution of dust ejected from the comet during post-di
scovery nuclear outbursts, and we consider the hypothetical nodal dist
ribution of meteoroids ejected from the comet during an assumed previo
us perihelion passage. In each case we find no reason to believe that
the Earth will sample any significant numbers of C/1995 01 derived met
eoroids.