Estimation of the dust mass-loss rates from AGB stars in the Fornax and Sagittarius dwarf spheroidal galaxies

被引:0
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作者
Lagadec, Eric [1 ]
Zijlstra, Albert A. [1 ]
Matsuura, M. [2 ]
Whitelock, Patricia A. [3 ]
van Loon, Jacco Th. [4 ]
机构
[1] Univ Manchester, Sch Phys & Astron, Sackville St Bldg,POB 88, Manchester M60 1QD, Lancs, England
[2] Natl Astron Observ Japan, Tokyo, Japan
[3] Univ Cape Town, Rondebosch, South Africa
[4] Univ Keele, Keele, Staffs, England
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P1 [天文学];
学科分类号
0704 ;
摘要
To study the effect of metallicity on the mass-loss of AGB stars, we have conducted mid-infrared photometric measurements of AGB stars in the Sagittarius and Fornax dwarf spheroidal galaxies ([Fe/H] = -1.1 and -1.3) with the 10 mu m camera VISIR at the VLT. These observations, combined with previous near-infrared photometric measurements, allow us to estimate mass-loss rates in these galaxies. We show here that the observed AGB stars display dust-driven mass-loss. Dust mass-loss rates are found to be in the range 6 x 10(-10) - 4.4 x 10(-8) M-circle dot yr(-1) for the observed AGB stars in SgrD and around 2 x 10(-8) M-circle dot yr(-1) for the star observed in Fornax.
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页码:268 / +
页数:3
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