Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars

We model the aspherical dust envelopes around O-rich AGB stars. We perform the radiative transfer model calculations for axisymmetric dust distributions. We simulate what could be observed from the aspherical dust envelopes around O-rich AGB stars by presenting the model spectral energy distribution...

Full description

Bibliographic Details
Main Author: Kyung-Won Suh
Format: Article
Language:English
Published: The Korean Space Science Society 2006-12-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2006/v23n4/OJOOBS_2006_v23n4_303.pdf
_version_ 1797331076187684864
author Kyung-Won Suh
author_facet Kyung-Won Suh
author_sort Kyung-Won Suh
collection DOAJ
description We model the aspherical dust envelopes around O-rich AGB stars. We perform the radiative transfer model calculations for axisymmetric dust distributions. We simulate what could be observed from the aspherical dust envelopes around O-rich AGB stars by presenting the model spectral energy distributions and images at various wavelengths for different optical depths and viewing angles. The model results are very different from the ones with spherically symmetric geometry.
first_indexed 2024-03-08T07:29:19Z
format Article
id doaj.art-8699b5968a0b476687e8d2b003e6ecd4
institution Directory Open Access Journal
issn 2093-5587
2093-1409
language English
last_indexed 2024-03-08T07:29:19Z
publishDate 2006-12-01
publisher The Korean Space Science Society
record_format Article
series Journal of Astronomy and Space Sciences
spelling doaj.art-8699b5968a0b476687e8d2b003e6ecd42024-02-02T20:54:40ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092006-12-0123430331010.5140/JASS.2006.23.4.303Aspherical Dust Envelopes Around Oxygen-Rich AGB StarsKyung-Won Suh0Department of Astronomy and Space Science, Chungbuk National University Cheongju 361-763, KoreaWe model the aspherical dust envelopes around O-rich AGB stars. We perform the radiative transfer model calculations for axisymmetric dust distributions. We simulate what could be observed from the aspherical dust envelopes around O-rich AGB stars by presenting the model spectral energy distributions and images at various wavelengths for different optical depths and viewing angles. The model results are very different from the ones with spherically symmetric geometry.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2006/v23n4/OJOOBS_2006_v23n4_303.pdfcircumstellar matterstars: AGB and post-AGBinfrared: starsdust: extinctionradiative transfer
spellingShingle Kyung-Won Suh
Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars
Journal of Astronomy and Space Sciences
circumstellar matter
stars: AGB and post-AGB
infrared: stars
dust: extinction
radiative transfer
title Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars
title_full Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars
title_fullStr Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars
title_full_unstemmed Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars
title_short Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars
title_sort aspherical dust envelopes around oxygen rich agb stars
topic circumstellar matter
stars: AGB and post-AGB
infrared: stars
dust: extinction
radiative transfer
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2006/v23n4/OJOOBS_2006_v23n4_303.pdf
work_keys_str_mv AT kyungwonsuh asphericaldustenvelopesaroundoxygenrichagbstars