Infrared diffuse interstellar bands

Г. А. Галазутдинов

doi:10.1093/mnras/stx330

2017-02-07

PRE

DOI：10.1093/mnras/stx330

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摘要

En 中文

We present high-resolution (R similar to 45000) profiles of 14 diffuse interstellar bands in the similar to 1.45 to similar to 2.45 mu m range based on spectra obtained with the Immersion Grating INfrared Spectrograph at the McDonald Observatory. The revised list of diffuse bands with accurately estimated rest wavelengths includes six new features. The diffuse band at 15 268.2 angstrom demonstrates a very symmetric profile shape and thus can serve as a reference for finding the 'interstellar correction' to the rest wavelength frame in the H range, which suffers from a lack of known atomic/molecular lines.

Keyword:

ISM: clouds

ISM: lines and bands

ISM: molecules

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期刊

Monthly Notices of the Royal Astronomical Society

IF:

4.8

论文数:

7.0W

被引数:

25.0W

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pulkovo observatory

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316

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russian academy of sciences

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9.1W

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被引数: 60

st. petersburg scientific centre of the russian academy of sciences

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3.6K

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universidad catolica del norte

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2.0K

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