A semi-empirical study of the mass distribution of horizontal branch stars in M 3 (NGC 5272)

Simple item page
dc.contributor.authorValcarce Bravo, Aldo Alfonso Raúl
dc.contributor.authorCatelan, Márcio
dc.date.accessioned2017-04-25T19:28:34Z
dc.date.available2017-04-25T19:28:34Z
dc.date.issued2008
dc.identifier.doi10.1051/0004-6361:20078231
dc.identifier.issn0004-6361
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/21021
dc.identifier.urihttps://doi.org/10.1051/0004-6361:20078231
dc.language.isoen
dc.relation.isformatofAstronomy & Astrophysics Vol. 487, no. 1 (2008), p. [185]-195
dc.revistaAstronomy & Astrophysicses_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas de ramaes_ES
dc.subject.otherEstrellas - Cúmuloes_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.subject.otherFotometría astronómicaes_ES
dc.titleA semi-empirical study of the mass distribution of horizontal branch stars in M 3 (NGC 5272)es_ES
dc.typeartículo
sipa.codpersvinculados16368
sipa.codpersvinculados1001556
Files
Original bundle
Now showing 1 - 1 of 1
Thumbnail Image
Name:
A semi-empirical study of the mass distribution of horizontal branch stars in M 3 (NGC 5272).pdf
Size:
1.06 MB
Format:
Adobe Portable Document Format
Description:
Download
Collections
Artículos de revistas