Oleg Egorov

Sep 17, 2024 | dx.doi.org | Oleg Egorov |Michael Rey

Sep 17, 2024 | pubs.acs.org | Oleg Egorov |Michael Rey

Aug 9, 2024 | dx.doi.org | Oleg Egorov |Michael Rey |Dominika Viglaska |Andrei V. Nikitin

Feb 23, 2024 | pubs.acs.org | Oleg Egorov |Johannes Beierlein |Philipp Gagel |Franciszek Dzimira

Download Hi-Res ImageDownload to MS-PowerPointCite This:Nano Lett. 2024, XXXX, XXX Terms & Conditions Most electronic Supporting Information files are available without a subscription to ACS Web Editions. Such files may be downloaded by article for research use (if there is a public use license linked to the relevant article, that license may permit other uses).

Oct 18, 2023 | aanda.org | Oleg Egorov |Astronomisches Rechen-Institut |Kathryn Kreckel |Brent Groves

We identify 1484 regions of locally elevated Hα velocity dispersion (σ(Hα) > 45 km s−1), with tens in each galaxy. About half of them contain at least one young stellar association or compact star cluster within their borders. We argue that most of those regions not connected with star clusters are SNRs – they typically have a centrally concentrated Hα flux distribution and emission line flux ratios consistent with shock excitation.