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dc.date.accessioned | 2020-03-31T13:59:10Z | |
dc.date.available | 2020-03-31T13:59:10Z | |
dc.date.issued | 1965 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/92443 | |
dc.description.abstract | The photoelectric observations made during the current year (1964) shows that all stars in a radius of 5' around η Carinae are members of the open cluster Trumpler 16. The brightest star, HD 93250, of spectral type 05 is on the zero age main sequence. One Wolf-Rayet star, HD 93162, would appear to be a member of the cluster, if we assume that besides the absorption of all the group, there is an additional absorption of Aᵥ=O.6 mag. With an extra color excess of E(B-V)= 0.2 mag, this star is in the color-magnitude diagram very near HD 93250. Then, its absolute magnitude is Mᵥ = -5.5. Other two stars in the cluster, CD -59.3308 deg and 331o, may also have some additional absorption of around Aᵥ= 0.3 mag. | en |
dc.language | es | es |
dc.subject | Galaxias | es |
dc.subject | η Carinae | es |
dc.title | El cúmulo abierto alrededor de la estrella η Carinae | es |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Feinstein, Alejandro | es |
sedici.subject.materias | Astronomía | es |
sedici.description.fulltext | true | es |
mods.originInfo.place | Asociación Argentina de Astronomía | es |
sedici.subtype | Comunicacion | es |
sedici.rights.license | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
sedici.rights.uri | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
sedici.relation.journalTitle | Boletín de la Asociación Argentina de Astronomía | es |
sedici.relation.journalVolumeAndIssue | no. 8, 9, 10 | es |