Bibcode
Tancredi, G.; Licandro, J.; Alí-Lagoa, V.; Martino, Silvia; Vieira Monteiro, Filipe; Silva, Jose Sergio; Lazzaro, Daniela
Referencia bibliográfica
IAU General Assembly, Meeting #29, #2255399
Fecha de publicación:
8
2015
Número de citas
0
Número de citas referidas
0
Descripción
The classification criterion between asteroids and comets has evolved in
recent decades, but the main phenomenological distinction remains
unchanged: comets are active objects as they present gas and dust
ejection from the surface at some point of their orbits, while asteroids
are inert objects as they do not show any kind of large scale gas and
dust ejection.To identify the transitional objects several
classification schemes based on the orbital elements have been used.
They are usually based on the Tisserand’s parameter (TJ). Tancredi
(2014) presents a much more restrictive criterion to identify ACOs that
ensured that the objects have a dynamical evolution similar to the
population of periodic comets. After applying the criteriaa to the
sample of over half a million asteroids already discovered, we obtain
316 ACOs that are further classified in subclasses similar to the
cometary classification: 203 objects belong to the Jupiter Family group;
72 objects are classified as Centaurs; and 56 objects have Halley Type
Orbits (also known as Damocloids). These are the best-known
extinct/dormant comets candidates from a dynamical point of view.We
study the physical properties of this sample of ACOs. Two results will
be presented:- We look for the ACOs detected by the NASA’s WISE
and by fitting a thermal model to their observations, we derive: the
effective diameter, beaming parameter and the visible geometric albedo,
using the method described in Al-Lagoa et al (2013). We obtain these
parameters for 37 of 203 ACOs in JFC orbits and 13 of 56 Damocloids. We
also compute the Cumulative Size Distribution (CSDs) of these
populations and compare them with the CSDs of JF Comets and Centaurs.-
We have been monitoring the observable ACOs since 12/2014 up to 06/2015.
Every other month we select all the ACOs with elongations >90deg and
estimated magnitudes V<21. We try to observe them with the 1m
IMPACTON telescope of the Observatório Astronômico do
Sertão de Itaparica (OASI). By comparing the photometric profiles
of the ACOs with background stars, we try to detect some hint of
cometary activity. Over 20 ACOs have been observed in the six months.