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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7931
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dc.contributor.authorDrozdov, Sergey A.-
dc.contributor.authorVasiliev, Evgenii O.-
dc.contributor.authorRyabova, Marina V.-
dc.contributor.authorShchekinov, Yuri A.-
dc.contributor.authorNath, Biman B.-
dc.date.accessioned2022-04-28T06:16:09Z-
dc.date.available2022-04-28T06:16:09Z-
dc.date.issued2022-04-13-
dc.identifier.citationOpen Astronomy, 2022, Vol. 31, p154en_US
dc.identifier.issn2543-6376-
dc.identifier.urihttp://hdl.handle.net/2289/7931-
dc.descriptionOpen Accessen_US
dc.description.abstractSupernovae explosions (SNe) in a stratified interstellar disc can create large scale structures and outflows perpendicular to the disc. Their morphology and emission characteristics depend on interrelations between the number of exploded SNe, the ISM vertical scale height, the height above the ISM disc at which SNe are located, and the mid-plane density of ambient gas. When observed such out-of-plane gas structures do characterize properties of the driving SNe and reveal the presence of underlying stellar clusters. Even though the morphology and emission properties of such structures are sensitive to characteristics of ambient gas they might be used for rough estimates of the clusters' mass.en_US
dc.language.isoenen_US
dc.publisherDe Gruyteren_US
dc.relation.urihttps://ui.adsabs.harvard.edu/abs/2022OAst...31..154D/abstracten_US
dc.relation.urihttps://doi.org/10.1515/astro-2022-0021en_US
dc.rights2022 Sergey A. Drozdov et alen_US
dc.subjectgalaxiesen_US
dc.subjectbubblesen_US
dc.subjectshock wavesen_US
dc.subjectsupernova remnantsen_US
dc.titleBubbles and OB associationsen_US
dc.typeArticleen_US
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