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ALMA Observation of Mass Loss from Massive Stars

Published online by Cambridge University Press:  28 July 2017

D. Y. A. Setia Gunawan
Affiliation:
IFA, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile
M. Curé
Affiliation:
IFA, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile
S. Kanaan
Affiliation:
IFA, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile
J. Puls
Affiliation:
LMU Munich, Universitäts-Sternwarte, Scheinerstr. 1, D-81679 München, Germany
F. Najarro
Affiliation:
Centro de Astrobiología (CSIC/INTA), 28850 Torrejón de Ardoz, Madrid, Spain
J. Sundqvist
Affiliation:
Centro de Astrobiología (CSIC/INTA), 28850 Torrejón de Ardoz, Madrid, Spain
M. M. Rubio Diez
Affiliation:
Centro de Astrobiología (CSIC/INTA), 28850 Torrejón de Ardoz, Madrid, Spain
N. Whyborn
Affiliation:
Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
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Abstract

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We present a pilot study of using the Atacama Large Millimeter/sub-millimeter Array (ALMA) continuum observations to constrain the density structure in the intermediate wind zone of massive stars, in which the wind is extremely sensitive to clumping.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017