RS Ophiuchi: differenze tra le versioni

Versione delle 23:54, 30 ott 2018

Versione delle 23:55, 30 ott 2018

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=====2006=====

L'esplosione del [[2006]], osservata per primo dall'astrofilo giapponese [[Hiroaki Narumi]], avvenne il 12 febbraio e raggiunse una magnitudine di 4,5.<ref>{{en}} [http://ooruri.kusastro.kyoto-u.ac.jp/mailarchive/vsnet-alert/8859 vsnet-alert 8859: RS Oph in outburst !!]</ref><ref>{{en}} [http://www.cbat.eps.harvard.edu/iauc/08600/08671.html IAUC 8671: N Oph 2006; RS Oph]</ref> Fu studiata in varie lunghezze d'onda <ref>{{en}} [https://arxiv.org/pdf/astro-ph/0607399.pdf NO EXPANDING FIREBALL: RESOLVING THE RECURRENT NOVA RS OPHIUCHI WITH INFRARED INTERFEROMETRY]</ref> <ref>{{en}} [https://arxiv.org/pdf/astro-ph/0604618.pdf Swift observations of the 2006 outburst of the recurrent nova RS Ophiuchi: I. Early X-ray emission from the shocked ejecta and red giant wind]</ref>.

INTERFEROMETRY]</ref> <ref>{{en}} [https://arxiv.org/pdf/astro-ph/0604618.pdf Swift observations of the 2006 outburst of the recurrent nova RS Ophiuchi: I. Early X-ray emission from the shocked ejecta and red giant wind]</ref>.

== Note ==