A 2010 superbolide produced by a meteoroid from a short period comet

dc.contributor.authorCruz, J.
dc.contributor.authorMadiedo Gil, José María
dc.contributor.authorOrtiz Moreno, José Luis
dc.contributor.authorCastro Tirado, Alberto J.
dc.contributor.authorTrigo Rodríguez, Josep María
dc.date.accessioned2014-10-29T10:26:11Z
dc.date.available2014-10-29T10:26:11Z
dc.date.issued2013
dc.description.abstractIn 2009 our team established a me- teor observing station in the Sierra Nevada Astronomi- cal Observatory (Granada, Spain), with the aim to monitor meteor and fireball activity over the south of the Iberian Peninsula and to develop a continuous me- teor spectroscopy campaign in the framework of the SPanish Meteor Network (SPMN). In this work, we analyze a very bri ght fireball that reached its maximum brightness next to the zenith of this observatory in 2010. In fact, with an absolute magnitude of about - 18, this event was classified as a superbolide
dc.description.departmentIngeniería Química, Química Física y Ciencias de los Materiales
dc.identifier.citationCruz, J., Madiedo Gil, J.M., Ortiz Moreno, J.L., Castro Tirado, Alberto J.: "A 2010 superbolide produced by a meteoroid from a short period comet". En: 44th Lunar and Planetary Science Conference (The Woolands, Texas, march 18-22, 2013)en_US
dc.identifier.urihttp://hdl.handle.net/10272/9010
dc.language.isoengen_US
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.accessRightsopen accessen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.titleA 2010 superbolide produced by a meteoroid from a short period cometen_US
dc.typeconference outputen_US
dspace.entity.typePublication
relation.isAuthorOfPublicatione4330c3a-5439-412d-a32d-970ba62002fd
relation.isAuthorOfPublication.latestForDiscoverye4330c3a-5439-412d-a32d-970ba62002fd

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