A Chandra Perspective on Galaxy-Wide X-ray Binary Emission and its Correlation with Star Formation Rate and Stellar Mass: New Results from Luminous Infrared Galaxies

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dc.contributor.authorLehmer, B. D.
dc.contributor.authorBauer, Franz Erik
dc.date.accessioned2016-05-10T18:02:10Z
dc.date.available2016-05-10T18:02:10Z
dc.date.issued2010
dc.identifier.doi10.1088/0004-637X/724/1/559
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/12128
dc.identifier.urihttps://doi.org/10.1088/0004-637X/724/1/559
dc.language.isoen
dc.relation.isformatofAstrophysical Journal No. 1 (724), p. 559-571.
dc.revistaAstrophysical Journales_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherGalaxiases_ES
dc.subject.otherFormación de Estrellases_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.titleA Chandra Perspective on Galaxy-Wide X-ray Binary Emission and its Correlation with Star Formation Rate and Stellar Mass: New Results from Luminous Infrared Galaxieses_ES
dc.typeartículo
sipa.codpersvinculados1007961
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