Observational studies on the near-infrared unidentified emission bands in galactic H II regions

Tamami I. Mori, Takashi Onaka, Itsuki Sakon, Daisuke Ishihara, Takashi Shimonishi, Ryou Ohsawa, Aaron C. Bell

研究成果: Article査読

19 被引用数 (Scopus)

抄録

Using a large collection of near-infrared spectra (2.5-5.4 μm) of Galactic H II regions and H II region-like objects, we perform a systematic investigation of astronomical polycyclic aromatic hydrocarbon (PAH) features. Thirty-six objects were observed using the infrared camera on board the AKARI satellite as a part of a director's time program. In addition to the well known 3.3-3.6 μm features, most spectra show a relatively weak emission feature at 5.22 μm with sufficient signal-to-noise ratios, which we identify as the PAH 5.25 μm band (previously reported). By careful analysis, we find good correlations between the 5.25 μm band and both the aromatic hydrocarbon feature at 3.3 μm and the aliphatic hydrocarbon features at around 3.4-3.6 μm. The present results give us convincing evidence that the astronomical 5.25 μm band is associated with C-H vibrations, as suggested by previous studies, and show its potential to probe the PAH size distribution. The analysis also shows that the aliphatic-to-aromatic ratio of I3.4-3.6 μm/I3.3 μm decreases against the ratio of the 3.7 μm continuum intensity to the 3.3 μm band, Icont, 3.7 μm/I 3.3 μm, which is an indicator of the ionization fraction of PAHs. The midinfrared color of I9μm/I18μm also declines steeply against the ratio of the hydrogen recombination line Brα at 4.05 μm to the 3.3 μm band, IBrα/I3.3 μm. These facts indicate possible dust processing inside or at the boundary of ionized gas.

本文言語English
論文番号53
ジャーナルAstrophysical Journal
784
1
DOI
出版ステータスPublished - 2014 3月 20

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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