Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-25T19:37:44.818Z Has data issue: false hasContentIssue false
  • English
  • Français

Dust Structure Around Asymptotic Giant Branch Stars – CORRIGENDUM

Published online by Cambridge University Press:  27 February 2020

D. Raj Upadhyay ,
L. Khanal ,
P. Hamal  and
B. Aryal
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The above article previously published with incorrect author information for Dr Binil Aryal. Dr Aryal’s affiliation should be listed as Central Department of Physics, Tribhuvan University, Kathmandu, Nepal. This error has since been rectified in the online PDF and HTML copies of the article.

Keywords

Stars: AGB and post-AGBmass-losscircumstellar matterdustISM: dustcorrigendum
Type
Corrigendum
Information
Proceedings of the International Astronomical Union , First View , pp. 1
Copyright
© International Astronomical Union 2020

References

Upadhyay, D., Khanal, L., Hamal, P., & Aryal, B. (2018). Dust Structure Around Asymptotic Giant Branch Stars. Proceedings of the International Astronomical Union, 14(S343), 525–526. doi:10.1017/S1743921318007858CrossRefGoogle Scholar