supported by a grant from the Israel Science Foundation(769/20)。
I present the effervescent zone model to account for the compact dense circumstellar material(CSM)around the progenitor of the core collapse supernova(CCSN)SN 2023ixf.The effervescent zone is composed of bound dense c...
supported by the Programme National "Physique et Chimie du MilieuInterstellaire" (PCMI) of CNRS/INSU with INC/INP co-funded by CEA and CNES;financial support from VNSC/VAST;the NAFOSTED funding agency under grant number 103.99–2015.39;the World Laboratory;the Odon Vallet Foundation;the Rencontres du Viet Nam;funded by Graduate University of Science and Technology undergrant number GUST.STS.DT 2017-VL01
Atacama Large Millimetre/sub-millimetre Array(ALMA) observations of CO(1–0) and CO(2–1) emissions from the circumstellar envelope of the asymptotic giant branch(AGB) star EP Aqr have been made with four times better...