Evolution of mid-infrared spectral energy distribution of dust forming nova V1280SCo based on infrared observations with subaru/COMICS, gemini/T-ReCS and AKARI/IRC

dc.contributor.authorSakon, I.
dc.contributor.authorSako, S.
dc.contributor.authorShimonishi, T.
dc.contributor.authoret al.
dc.date.accessioned2012-03-06T03:31:56Z
dc.date.available2012-03-06T03:31:56Z
dc.date.issued2011-11-22
dc.identifier.urihttp://hdl.handle.net/11007/533
dc.language.isoenen_US
dc.relation.ispartofseriesInternational conference on interstellar dust, molecules and chemistry, IUCAA, Pune, India (Nov.2011);
dc.subjectSpectral energyen_US
dc.subjectDust formingen_US
dc.subjectPPTen_US
dc.subjectV1280SCoen_US
dc.subjectCOMICSen_US
dc.subjectGemini/T-ReCSen_US
dc.subjectAKARI/IRCen_US
dc.titleEvolution of mid-infrared spectral energy distribution of dust forming nova V1280SCo based on infrared observations with subaru/COMICS, gemini/T-ReCS and AKARI/IRCen_US
dc.typePresentationen_US

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