Figure 1 - uploaded by Thomas I. Maindl
Content may be subject to copyright.
Source publication
67P/Churyumov-Gerasimenko is a bi-lobed comet connected by a thick neck. The aim of our work is to find the possible origins of this comet, dynamically and physically.
Similar publications
Kuiper-like belts of planetesimals orbiting stars other than the Sun are most commonly detected from the thermal emission of small dust produced in collisions. Emission from gas, most notably CO, highlights the cometary nature of these planetesimals. Here we present models for the release of gas from comet-like bodies in these belts, both due to th...
