WHAT IS THE DIFFERENCE? BLAZHKO AND NON-BLAZHKO RRab STARS AND THE SPECIAL CASE OF V123 IN M3

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dc.contributor.authorJurcsik, J.
dc.contributor.authorHajdu, Gergely
dc.date.accessioned10-05-2016 15:16
dc.date.available10-05-2016 15:16
dc.date.issued2013
dc.identifier.doi10.1088/2041-8205/778/2/L27
dc.identifier.issn2041-8205
dc.identifier.urihttps://doi.org/10.1088/2041-8205/778/2/L27
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/14337
dc.identifier.wosidWOS:000327428400005
dc.language.isoen
dc.nota.accesoContenido completo
dc.relation.isformatofThe Astrophysical Journal Letters No. 2 (778), p. 1-5.
dc.revistaThe Astrophysical Journal Letters
dc.subject.ddc520
dc.subject.deweyAstronomía
dc.subject.otherEstrellas - Cúmulos globulares
dc.subject.otherEstrellas variables
dc.subject.otherEstrellas RR Lyr
dc.titleWHAT IS THE DIFFERENCE? BLAZHKO AND NON-BLAZHKO RRab STARS AND THE SPECIAL CASE OF V123 IN M3
dc.typeartículo
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