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Modelling dust around Nearby Evolved Stars Survey (NESS) Targets

Published online by Cambridge University Press:  30 December 2019

Sundar Srinivasan
Affiliation:
Academia Sinica Institute of Astronomy & Astrophysics (ASIAA) 11F Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan email: [email protected]
T. Dharmawardena
Affiliation:
Academia Sinica Institute of Astronomy & Astrophysics (ASIAA) 11F Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan email: [email protected]
F. Kemper
Affiliation:
Academia Sinica Institute of Astronomy & Astrophysics (ASIAA) 11F Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan email: [email protected]
P. Scicluna
Affiliation:
Academia Sinica Institute of Astronomy & Astrophysics (ASIAA) 11F Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan email: [email protected]
The NESS Collaboration
Affiliation:
Academia Sinica Institute of Astronomy & Astrophysics (ASIAA) 11F Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Road, Taipei 10617, Taiwan email: [email protected]
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Abstract

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We present radiative transfer modelling of the dust around U Ant, a well-studied detached-shell source. U Ant is among the >400 sources targeted by the Nearby Evolved Stars Survey (NESS; PI: P. Scicluna), and the procedure used to model this source will be applied to the rest of the AGB sample in NESS.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

Footnotes

Present address: Instituto de Radioastronomía y Astrofísica, Universidad Nacional Autonóma de México, Antigua Carretera a Pátzcuaro #8701, Ex-Hda. San José de La Huerta, Morelia, Michoacán, 58089, México.

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