An Upper Bound to the Space Density of Interstellar Comets

Details An Upper Bound to the Space Density of Interstellar Comets An Upper Bound to the Space Density of Interstellar Comets

2011-02-21

arxiv.org/abs/1102.4319v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

Astronomical Journal, accepted

Scientific paper

Two well-studied white dwarfs with helium-dominated atmospheres (DBs) each possess less hydrogen than carried by a single average-mass comet. Plausibly, the wind rates from these stars are low enough that most accreted hydrogen remains with the star. If so, and presuming their nominal effective temperatures, then these DBs have been minimally impacted by interstellar comets during their 50 Myr cooling age; interstellar iceballs with radii between 10 m and 2 km contain less than 1% of all interstellar oxygen. This analysis suggests that most stars do not produce comets at the rate predicted by "optimistic" scenarios for the formation of the Oort cloud.

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