2014A&A...566A..69M


C.D.S. - SIMBAD4 rel 1.7 - 2020.02.24CET09:54:24

2014A&A...566A..69M - Astronomy and Astrophysics, volume 566A, 69-69 (2014/6-1)

Dusty shells surrounding the carbon variables S Scuti and RT Capricorni.

MECINA M., KERSCHBAUM F., GROENEWEGEN M.A.T., OTTENSAMER R., BLOMMAERT J.A.D.L., MAYER A., DECIN L., LUNTZER A., VANDENBUSSCHE B., POSCH Th. and WAELKENS C.

Abstract (from CDS):

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 70µm and 160µm 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.

Abstract Copyright:

Journal keyword(s): stars: AGB and post-AGB - stars: carbon - stars: mass-loss - infrared: stars - stars: individual: S Sct - stars: individual: RT Cap

Simbad objects: 7

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Number of rows : 7

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 V* R Scl C* 01 26 58.0946233986 -32 32 35.437732667 17.26 9.59 5.72 3.69 2.30 C-N5+ 293 0
2 * omi Cet Mi* 02 19 20.79210 -02 58 39.4956   7.63 6.53 5.03   M5-9IIIe+DA 1422 0
3 V* U Cam C* 03 41 48.1762532767 +62 38 54.397016016   11.5 11.00     C-N5 230 0
4 V* Y CVn C* 12 45 07.8257032577 +45 26 24.898861195 14.03 7.41 4.87 3.12 1.74 C-N5 460 0
5 V* S Sct C* 18 50 20.0367524071 -07 54 27.430964220 13.93 9.89 6.80     C-N5 194 0
6 V* TT Cyg C* 19 40 57.0159854799 +32 37 05.755486755   10.43 10.20     C-N5- 185 0
7 V* RT Cap C* 20 17 06.5288478069 -21 19 04.462721142   12.92 8.90     C6,4 113 0

    Equat.    Gal    SGal    Ecl

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2020.02.24-09:54:24

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