Open AccessThree-dimensional Monte Carlo dust radiative transfer study of the H-poor planetary nebula IRAS 18333–2357 located in M22
Author(s) -
C. Muthumariappan
Publication year - 2017
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stx1071
Subject(s) - physics , planetary nebula , astrophysics , radiative transfer , nebula , spectral energy distribution , luminosity , population , asymptotic giant branch , carbon star , amorphous carbon , circumstellar dust , atmospheric radiative transfer codes , reflection nebula , astronomy , cosmic dust , stars , galaxy , demography , sociology , raman spectroscopy , quantum mechanics , optics
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