RT Journal Article
T1 Analysis of the September ε-Perseid outburst in 2013
A1 Madiedo Gil, José María
A1 Pujols, P.
AB We analyse the outburst experienced by the September ε-Perseid meteor shower on 2013 September 9. As a result of our monitoring, the atmospheric trajectory of 60 multistation events observed over Spain was obtained and accurate orbital data were derived from them. On the basis of these orbits, we have tried to determine the likely parent body of this meteoroid stream by employing orbital dissimilarity criteria. In addition, the emission spectra produced by two events belonging to this meteor shower were also recorded. The analysis of these spectra has provided information about the chemical nature of their progenitor meteoroids. We also present an estimation of the tensile strength for these particles.
PB Oxford University Press
SN 0035-8711
SN 1365-2966 (electrónico)
YR 2018
FD 2018
LK http://hdl.handle.net/10272/15192
UL http://hdl.handle.net/10272/15192
LA eng
NO Madiedo, J. M., Zamorano, J., Trigo-Rodríguez, J. M., Ortiz, J. L., Docobo, J. A., Izquierdo, J., … Pujols, P. (2018). Analysis of the September ε-Perseid outburst in 2013. Monthly Notices of the Royal Astronomical Society, 480(2), 2501-2507. https://doi.org/10.1093/mnras/sty1973
NO We acknowledge support from the Spanish Ministry of Science and Innovation (projectsAYA2015-68646-P and AYA 2015-67175-P).
DS Repositorio Institucional de la Universidad de Huelva
RD 1 jun 2026