A Survey of Near-infrared Diffuse Interstellar Bands | Zendy

Satoshi Hamano | Zendy; Naoto Kobayashi | Zendy; Hideyo Kawakita | Zendy; Yuji Ikeda | Zendy; Sohei Kondo | Zendy; Hiroaki Sameshima | Zendy; Akira Arai | Zendy; Noriyuki Matsunaga | Zendy; Chikako Yasui | Zendy; Misaki Mizumoto | Zendy; Kei Fukue | Zendy; Natsuko Izumi | Zendy; Shogo Otsubo | Zendy; Keiichi Takenaka | Zendy

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A Survey of Near-infrared Diffuse Interstellar Bands

Author(s) -

Satoshi Hamano,

Naoto Kobayashi,

Hideyo Kawakita,

Yuji Ikeda,

Sohei Kondo,

Hiroaki Sameshima,

Akira Arai,

Noriyuki Matsunaga,

Chikako Yasui,

Misaki Mizumoto,

Kei Fukue,

Natsuko Izumi,

Shogo Otsubo,

Keiichi Takenaka

Publication year - 2018

Publication title -

bulletin de la société royale des sciences de liège

Language(s) - English

Resource type - Journals

ISSN - 1783-5720

DOI - 10.25518/0037-9565.7702

Subject(s) - spectrograph , physics , near infrared spectroscopy , astrophysics , telescope , stars , spectroscopy , astronomy , spectral resolution , interstellar medium , interstellar cloud , wavelength , infrared , spectral line , molecular cloud , optics , galaxy

Diffuse interstellar bands (DIBs) are ubiquitous absorption lines in the spectra of the reddened stars, which originate from foreground interstellar clouds. Although the carriers of most DIBs have not been successfully identified yet, they are considered to arise from the gas-phase carbonaceous molecules, such as fullerenes, polycyclic aromatic hydrocarbons (PAHs) and carbon-chain molecules [1]. The observational studies of DIBs may play an important role toward the understanding of the properties and chemistry of large organic molecules in interstellar medium.

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