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Relations between column densities of OH+, OH+ and CH+ molecules and between atomic and molecular hydrogen and intensities of major 5780 Å and 5797 Å diffuse interstellar bands are examined based on spectra of 46 stars. Data on OH+, OH, CH+ and atomic/molecular hydrogen were taken from the literature. Data on 5780 Å and 5797 Å DIBs are based mostly on our own measurements. Column densities of the OH+ are very well correlated with abundances of OH molecule and not correlated with CH+ and hydrogen in any form. Column densities of OH+ are better correlated with narrow 5797 Å than 5780 Å major DIB. The value of abundance ratio in the case of OH and OH+ molecules in the ISM is equal to 5.73±0.45.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
301--312
Opis fizyczny
Bibliogr. 62 poz., rys., tab.
Twórcy
autor
- Institute of Physics, Kazimierz Wielki University, ul. Weyssenhoffa 11, 85-072 Bydgoszcz, Poland
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-ec1ee979-c17c-48cb-9ea5-08865df90968