Diffuse interstellar bands towards ο Per and ξ Per

Spectroscopic characteristics of interstellar matter vary strongly with the direction to the target star. Spectra of oPer and ξ Per contain many prominent and weak diffuse interstellar bands as well as absorption lines of some identiffed interstellar atoms and molecules. Using echelle optical spectr...

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Bibliographic Details
Published in:Advances in Astronomy and Space Physics
Date:2012
Main Authors: Debudej, A., Kusiak, S., Ozga, J., Wszołek, B.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2012
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119148
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Diffuse interstellar bands towards ο Per and ξ Per / A. Debudej, S. Kusiak, J. Ozga, B. Wszołek // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 36-38. — Бібліогр.: 5 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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Summary:Spectroscopic characteristics of interstellar matter vary strongly with the direction to the target star. Spectra of oPer and ξ Per contain many prominent and weak diffuse interstellar bands as well as absorption lines of some identiffed interstellar atoms and molecules. Using echelle optical spectra of these bright and moderately reddened stars we selected well detectable diffuse interstellar bands (DIBs). We measured intensities of all well noticeable absorption features to compare them with their counterparts observed in spectra of the other target stars.
ISSN:2227-1481