@conference{10272/9389,
year = {2013},
url = {http://hdl.handle.net/10272/9389},
abstract = {The Geminids is the densest annual
meteoroid stream whose parent body is asteroid (3200)
Phaethon, which was considered by some researchers
as an extinct cometary nucleus rather than a regular
asteroid [1]. On the basis of spectral and dynamical
similarities, it has been recently proposed that asteroid
2 Pallas is the likely parent body of asteroid (3200)
Phaeton [2, 3]. The asteroidal origin of the Geminids
suggests that this stream could be a potential meteorite
producer. The analysis of several Geminid fireballs
observed between 2009 and 2010 from Spain supports
this idea [4]. In this work we present the preliminary
analysis of four emission spectra produced by meteoroids
from the Geminids stream. These were obtained
in the framework of the continuous spectroscopic campaign
developed by the SPanish Meteor Network
(SPMN).},
title = {Spectra of bolides produced by meteoroids from (3200) phaeton},
author = {Moreno, A. and Madiedo Gil, José María and Trigo Rodríguez, Josep María},
}