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Interstellar and circumstellar medium in the direction to IR source IRAS 01005+7910

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Abstract

Using the high-resolution spectra obtained at the 6-meter telescope of the SAO RAS over 2002–2013, we studied the spectral features of the lines of interstellar medium. The radial velocities of the Na I 5890 Å, Na I 5896 Å, Ca II 3934 Å and Ca II 3968 Å absorption lines were analyzed. Seven diffuse interstellar bands 4964, 5780, 5797, 6196, 6203, 6379 Å were identified in the optical spectrum of IRAS01005+7910. Radial velocities V r and equivalent widths W λ of these DIBs were measured, for which the values of the interstellar reddening E B−V and column density of neutral hydrogen log [N(H)] were calculated.

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Authors and Affiliations

  1. Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, 369167, Russia

    E. G. Sendzikas

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  1. E. G. Sendzikas
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Correspondence to E. G. Sendzikas.

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Original Russian Text © E.G. Sendzikas, 2016, published in Astrofizicheskii Byulleten, 2016, Vol. 71, No. 1, pp. 80–87.

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Sendzikas, E.G. Interstellar and circumstellar medium in the direction to IR source IRAS 01005+7910. Astrophys. Bull. 71, 75–81 (2016). https://doi.org/10.1134/S1990341316010089

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  • DOI: https://doi.org/10.1134/S1990341316010089

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