Mass Loss History of the AGB star, R Cas

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dc.creatorUeta, Toshiya
dc.creatorStencel, Robert E.
dc.creatorYamamura, Issei
dc.creatorIzumiura, Hideyuki
dc.creatorNakada, Yoshikazu
dc.creatorMatsuura, Mikako
dc.creatorIta, Yoshifusa
dc.creatorTanabe, Toshihiko
dc.creatorFukushi, Hinako
dc.creatorMatsunaga, Noriyuki
dc.creatorMito, Hiroyuki
dc.creatorSpeck, Angela K.
dc.date2009-05-06
dc.date.accessioned2026-07-07T13:12:11Z
dc.date.available2026-07-07T13:12:11Z
dc.descriptionWe report here on the discovery of an extended far-infrared shell around the AGB star, R Cassiopeia, made by AKARI and Spitzer. The extended, cold circumstellar shell of R Cas spans nearly 3 arcmin and is probably shaped by interaction with the interstellar medium. This report is one of several studies of well-resolved mass loss histories of AGB stars under AKARI and Spitzer observing programs labeled "Excavating Mass Loss History in Extended Dust Shells of Evolved Stars (MLHES)".
dc.descriptionPoster contribution, to be published in the proceedings of the conference "AKARI, a light to illuminate the misty Universe" held at University of Tokyo, Japan, 16-19 February 2009
dc.identifierhttps://arxiv.org/abs/0905.0750
dc.identifierhttp://arxiv.org/abs/0905.0750
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229509
dc.subjectAstrophysics of Galaxies
dc.titleMass Loss History of the AGB star, R Cas
dc.typetext

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