Near-infrared diffuse interstellar bands in 0.91-1.32 micron

We present a comprehensive survey of diffuse interstellar bands (DIBs) in \(0.91-1.32\mu\)m with a newly-developed near-infrared (NIR) spectrograph, WINERED, mounted on the Araki 1.3 m Telescope in Japan. We obtained high-resolution (\(R=28,300\)) spectra of 25 early-type stars with color excesses o...

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Bibliographic Details
Published in:arXiv.org 2015-02
Main Authors: Hamano, Satoshi, Kobayashi, Naoto, Kondo, Sohei, Ikeda, Yuji, Nakanishi, Kenshi, Yasui, Chikako, Mizumoto, Misaki, Matsunaga, Noriyuki, Fukue, Kei, Mito, Hiroyuki, Yamamoto, Ryo, Izumi, Natsuko, Nakaoka, Tetsuya, Kawanishi, Takafumi, Kitano, Ayaka, Otsubo, Shogo, Kinoshita, Masaomi, Kobayashi, Hitomi, Kawakita, Hideyo
Format: Article
Language:English
Subjects:
Cations
Chemical reactions
Correlation analysis
Diffuse interstellar bands
Interstellar matter
Ionization potentials
Near infrared radiation
Organic chemistry
Physical properties
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Summary:We present a comprehensive survey of diffuse interstellar bands (DIBs) in \(0.91-1.32\mu\)m with a newly-developed near-infrared (NIR) spectrograph, WINERED, mounted on the Araki 1.3 m Telescope in Japan. We obtained high-resolution (\(R=28,300\)) spectra of 25 early-type stars with color excesses of \(0.07
ISSN:2331-8422
DOI:10.48550/arxiv.1412.3578