activity
19992024
most citedInterstellar OH+, H2O+ and H3O+ along the sight-line to G10.6-0.4

185 citations · 1.1k across the 27 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2024★ 6 cited

Position displacement of diffuse interstellar bands

G. Galazutdinov, J. Krełowski, Y. Beletsky +1

We re-consider the already published phenomenon: the blue shift of diffuse interstellar bands, observed in spectra of HD34078 (AE Aur) and members of the Sco OB1 association, in pa…

astro-ph.GA2023★ 7 cited

Dark Dust III: The high-quality single-cloud reddening curve sample. Scrutinizing extinction curves in the Milky Way

R. Siebenmorgen, J. Smoker, J. Krełowski +2

The nature of dust in the diffuse interstellar medium can be best investigated by means of reddening curves where only a single interstellar cloud lies between the observer and the…

astro-ph.GA2022★ 7 cited

Broadened profiles of Diffuse Interstellar Bands

J. Krełowski, G. A. Galazutdinov, P. Gnaciński +3

The paper describes profile broadening and peak wavelength variation of diffuse interstellar bands (DIBs) measured for 46 lines of sight, probably caused by physical properties of…

astro-ph.GA2021★ 17 cited

Diffuse bands 9577 and 9633 -- relations to other interstellar features

G. A. Galazutdinov, G. Valyavin, N. R. Ikhsanov +1

We study, for the first time, the relations of two strong diffuse bands (DIBs) at 9633 and 9577~Å, commonly attributed to C, to other interstellar features seen in optical…

astro-ph.GA2020★ 20 cited

Dark Dust and single-cloud sightlines in the ISM

R. Siebenmorgen, J. Krełowski, J. Smoker +2

The precise characteristics of clouds and the nature of dust in the diffuse interstellar medium can only be extracted by inspecting the rare cases of single-cloud sightlines. In ou…

astro-ph.GA2020★ 16 cited

Survey of very broad Diffuse Interstellar Bands

G. Galazutdinov, A. Bondar, Byeong-Cheol Lee +3

This paper considers a very special set of a few interstellar features --- broad diffuse interstellar bands (DIBs) at 4430, 4882, 5450, 5779 and 6175 ÅÅ. The set is small, and meas…