Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/290
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dc.contributor.authorArbutina, Bojanen_US
dc.contributor.authorUrošević, Dejanen_US
dc.contributor.authorVukotić, B.en_US
dc.date.accessioned2022-08-06T17:48:13Z-
dc.date.available2022-08-06T17:48:13Z-
dc.date.issued2006-08-01-
dc.identifier.issn17439213en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/290-
dc.description.abstractIt is a general belief that the starburst activity of a nearby galaxy M82 was triggered in a close encounter with its massive companion M81, a few tens of million years ago. Despite the lack of supernovae observed, multiwavelength radio observations of M82 discovered a considerable number of compact supernova remnant candidates. We use these remnants to estimate the supernova rate (SNR) and the enhanced star-formation (SFR) rate in M82, and compare them with rates in normal galaxies. © 2007 International Astronomical Union.en
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.titleHigh supernova rate and enhanced star-formation triggered in M81-M82 encounteren_US
dc.typeConference Paperen_US
dc.relation.publicationTriggered Star Formation in a Turbulent ISMen_US
dc.identifier.doi10.1017/S1743921307001792-
dc.identifier.scopus2-s2.0-37049013123-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/37049013123-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage391en_US
dc.relation.volume2en_US
dc.relation.issueS237en_US
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-8036-4132-
crisitem.author.orcid0000-0003-0665-0939-
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