DC Field | Value | Language |
---|---|---|
dc.contributor.author | Pavlović, Marina | en_US |
dc.contributor.author | Prodanović, Tijana | en_US |
dc.date.accessioned | 2020-12-16T11:40:12Z | - |
dc.date.available | 2020-12-16T11:40:12Z | - |
dc.date.issued | 2019 | - |
dc.identifier.issn | 0352-4906 | - |
dc.identifier.uri | http://researchrepository.mi.sanu.ac.rs/handle/123456789/4510 | - |
dc.description.abstract | Far infrared-radio correlation represents a linear relationship between far-infrared (FIR) and radio emission in star-forming galaxies. Previous observations have confirmed that this correlation is maintained over a large range of redshift and does not evolve, although a small dispersion is present. However, some of more recent observations at high redshift have shown the opposite. The question that arises is - what is driving this evolution? In this paper we investigate the possibility that galaxy morphology is the answer to this question. A sample of 37 submillimeter galaxies (SMGs) is analyzed. The observation and morphological class of these galaxies has previously been published. We examined FIR-radio correlation in galaxies of different morphological type in this sample and found that for star-forming disk galaxies correlation is stable and does not evolve and for irregular and interacting galaxies we find some hints of evolution. | en_US |
dc.publisher | Matica srpska, Novi Sad | en_US |
dc.relation.ispartof | Zbornik Matice srpske za prirodne nauke | en_US |
dc.subject | cosmic rays | galaxy evolution | interactions of galaxies | infrared: galaxies | radio continuum: galaxies | en_US |
dc.title | What is driving the evolution of the far-infrared radio correlation? | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.2298/ZMSPN1937009P | - |
dc.relation.firstpage | 9 | - |
dc.relation.lastpage | 16 | - |
dc.relation.volume | 137 | - |
dc.description.rank | М51 | - |
item.grantfulltext | none | - |
item.cerifentitytype | Publications | - |
item.fulltext | No Fulltext | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
crisitem.author.orcid | 0000-0001-5560-7051 | - |
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