@conference{10272/9356,
year = {2013},
url = {http://hdl.handle.net/10272/9356},
abstract = {The first observations of meteor activity
in July from a radiant in the vicinity of Deneb
were performed by Denning between 1885 and 1918
[1]. This minor shower, that was called the omicron-
Cygnids, was described in detail by Jenniskens [2],
who determined an entry velocity for meteoroids of
about 37 km/s and a radiant located at α=305º, δ=47º.
In a latter paper by Olech et al [3], the activity period
of the omicron-Cygnids was determined to extend
from around June 30 to July 31, with a clear maximum
near July 18 and an entry velocity of meteoroids of
about 41 km/s. In any event, our knowledge about the
omicron-Cygnids is poor. Thus, observations during
the activity period of this shower are desirable in order
to obtain precise orbital information, but also to determine
different physico-chemical properties of meteoroids
in this stream. In particular, meteor spectroscopy
can be very useful to obtain information about the
chemical nature of these particles. In this context, we
present here the analysis of an omicron Cygnid fireball
recorded in the framework of the SPanish Meteor
Network (SPMN) in 2012},
title = {Orbital parameters and chemical nature of omicron cygnids meteoroids},
author = {Jiménez, P. and Madiedo Gil, José María and Trigo Rodríguez, Josep María},
}