TY - JOUR
T1 - Dusty shells surrounding the carbon variables S Scuti and RT Capricorni
AU - Mecina, Marko
AU - Kerschbaum, Franz
AU - Groenewegen, Martin A. T.
AU - Ottensamer, Roland
AU - Mayer, Andreas
AU - Luntzer, Armin
AU - Posch, Thomas
AU - Blommaert, Joris A D L
AU - Decin, Leen
AU - Vandenbussche, Bart
AU - Waelkens, Christoffel
PY - 2014/6
Y1 - 2014/6
N2 - For the Mass-loss of Evolved StarS (MESS) programme, the unprecedented spatial resolution of the PACS photometer on board the Herschel Space Observatory was employed to map the dusty environments of asymptotic giant branch (AGB) and red supergiant (RSG) stars. Among the morphologically heterogeneous sample, a small fraction of targets is enclosed by spherically symmetric detached envelopes. Based on observations in the 70 μm and 160 μm wavelength bands, we investigated the surroundings of the two carbon semiregular variables S Sct and RT Cap, which both show evidence for a history of highly variable mass-loss. S Sct exhibits a bright, spherically symmetric detached shell, 138″ in diameter and co-spatial with an already known CO structure. Moreover, weak emission is detected at the outskirts, where the morphology seems indicative of a mild shaping by interaction of the wind with the interstellar medium, which is also supported by the stellar space motion. Two shells are found around RT Cap that were not known so far in either dust emission or from molecular line observations. The inner shell with a diameter of 188″ shows an almost immaculate spherical symmetry, while the outer ~5′ structure is more irregularly shaped. MoD, a modification of the DUSTY radiative transfer code, was used to model the detached shells. Dust temperatures, shell dust masses, and mass-loss rates are derived for both targets.
AB - For the Mass-loss of Evolved StarS (MESS) programme, the unprecedented spatial resolution of the PACS photometer on board the Herschel Space Observatory was employed to map the dusty environments of asymptotic giant branch (AGB) and red supergiant (RSG) stars. Among the morphologically heterogeneous sample, a small fraction of targets is enclosed by spherically symmetric detached envelopes. Based on observations in the 70 μm and 160 μm wavelength bands, we investigated the surroundings of the two carbon semiregular variables S Sct and RT Cap, which both show evidence for a history of highly variable mass-loss. S Sct exhibits a bright, spherically symmetric detached shell, 138″ in diameter and co-spatial with an already known CO structure. Moreover, weak emission is detected at the outskirts, where the morphology seems indicative of a mild shaping by interaction of the wind with the interstellar medium, which is also supported by the stellar space motion. Two shells are found around RT Cap that were not known so far in either dust emission or from molecular line observations. The inner shell with a diameter of 188″ shows an almost immaculate spherical symmetry, while the outer ~5′ structure is more irregularly shaped. MoD, a modification of the DUSTY radiative transfer code, was used to model the detached shells. Dust temperatures, shell dust masses, and mass-loss rates are derived for both targets.
KW - Infrared: stars
KW - Stars: AGB and post-AGB
KW - Stars: carbon
KW - Stars: individual: RT Cap
KW - Stars: individual: S Sct
KW - Stars: mass-loss
UR - http://www.scopus.com/inward/record.url?scp=84902529136&partnerID=8YFLogxK
U2 - 10.1051/0004-6361/201321117
DO - 10.1051/0004-6361/201321117
M3 - Article
VL - 566
JO - Astronomy & Astrophysics
JF - Astronomy & Astrophysics
SN - 0004-6361
M1 - A69
ER -