천문학회지 (Journal of The Korean Astronomical Society)

  • 제37권4호
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  • Pages.289-294
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  • 2004
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  • 1225-4614(pISSN)
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  • 2288-890X(eISSN)
한국천문학회 (The Korean Astronomical Society)
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DUST GRAINS IN AGB STARS AS SOURCES OF INTERSTELLAR DUST

  • SUH KYUNG- WON (Department of Astronomy & Space Science, Chungbuk National University Cheongju-City)
  • 발행 : 2004.12.01
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초록

The main sources of interstellar dust are believed to be dust envelopes around AGB stars. The outflowing envelopes around the long period pulsating variables are very suitable place for massive dust formation. Oxygen-rich silicate dust grains or carbon-rich dust grains form in the envelopes around AGB stars depending on the chemical composition of the stellar surface. The dust grains expelled from AGB stars get mixed up and go through some physical and chemical changes in interstellar medium. There are similarities and differences between interstellar dust and dust grains in AGB stars. The mass cycle in the Galaxy may be best manifested by the fact that the dust grains at various regions have many similarities and understandable differences.

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피인용 문헌

  1. Infrared nebulae around bright massive stars as indicators for binary interactions vol.618, pp.1432-0746, 2018, https://doi.org/10.1051/0004-6361/201832722