Please use this identifier to cite or link to this item:
https://research.matf.bg.ac.rs/handle/123456789/1454
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Lalović, A | en_US |
dc.contributor.author | Petraš, Ivan | en_US |
dc.contributor.author | Jovanović, Milan | en_US |
dc.contributor.author | Knežević, Sladjana | en_US |
dc.contributor.author | Samurović, S | en_US |
dc.date.accessioned | 2025-02-12T14:06:56Z | - |
dc.date.available | 2025-02-12T14:06:56Z | - |
dc.date.issued | 2022 | - |
dc.identifier.uri | https://research.matf.bg.ac.rs/handle/123456789/1454 | - |
dc.language.iso | en | en_US |
dc.publisher | Edp Sciences | en_US |
dc.relation.ispartof | Astronomy and Astrophysics | en_US |
dc.title | Implications of the correlation between bulge-to-total baryonic mass ratio and the number of satellites for SAGA galaxiess ratio | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1051/0004-6361/202243286 | - |
dc.identifier.scopus | 2-s2.0-85131441227 | - |
dc.identifier.isi | 000804860900001 | - |
dc.identifier.url | https://www.aanda.org/articles/aa/pdf/2022/06/aa43286-22.pdf | - |
dc.identifier.url | http://dx.doi.org/10.1051/0004-6361/202243286 | - |
dc.contributor.affiliation | Astronomy | en_US |
dc.relation.issn | 0004-6361 | en_US |
dc.description.rank | М21 | en_US |
dc.relation.firstpage | Article no. A17 | en_US |
dc.relation.volume | 662 | en_US |
item.languageiso639-1 | en | - |
item.grantfulltext | none | - |
item.fulltext | No Fulltext | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | Astronomy | - |
crisitem.author.orcid | 0009-0003-9220-4093 | - |
Appears in Collections: | Research outputs |
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