천문학논총 (Publications of The Korean Astronomical Society)

  • 제32권1호
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  • Pages.93-95
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  • 2017
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  • 1225-1534(pISSN)
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  • 2287-6936(eISSN)
한국천문학회 (The Korean Astronomical Society)
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MODELLING THE 3 MICRON REGION IN AKARI IRC SPECTRA

  • 투고 : 2015.12.27
  • 심사 : 2016.10.21
  • 발행 : 2017.03.31
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초록

The existence of polycyclic aromatic hydrocarbons (PAHs) astronomically is well accepted, but the specific molecular forms observed remain uncertain. To better understand the molecular structures which may be present along a given sightline, the $3.0-3.6{\mu}m$ region is modelled with careful consideration given to the underlying sub-features arising from specific structures within emitting molecules.

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참고문헌

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