Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Piatti, Andres Eduardo | - |
| dc.date | 2017-07-03T17:39:02Z | - |
| dc.date | 2017-07-03T17:39:02Z | - |
| dc.date | 2012-06 | - |
| dc.date | 2017-06-30T17:28:23Z | - |
| dc.date.accessioned | 2019-04-29T15:32:45Z | - |
| dc.date.available | 2019-04-29T15:32:45Z | - |
| dc.date.issued | 2017-07-03T17:39:02Z | - |
| dc.date.issued | 2017-07-03T17:39:02Z | - |
| dc.date.issued | 2012-06 | - |
| dc.date.issued | 2017-06-30T17:28:23Z | - |
| dc.identifier | Piatti, Andres Eduardo; Astrophysical properties of star fields in the Large Magellanic Cloud; Asociación Argentina de Astronomía; Boletín de la Asociación Argentina de Astronomía; 55; 6-2012; 329-332 | - |
| dc.identifier | 0571-3285 | - |
| dc.identifier | http://hdl.handle.net/11336/19392 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/296195 | - |
| dc.description | We present CCD Washington CT1 photometry for the unprecedented database of some 5.5 million of stars distributed throughout the entire Large Magellanic Cloud (LMC) main body. The quality and performance of the data were rigurously examined from extensive completeness artificial star tests over the whole mosaic image data set, so that field colour-magnitude diagrams (CMDs) were accurately produced. From the star field CMD Hess diagrams, we identified the peaks at the main -sequence turnoff and red clump locations to date the most dominant sub-population (or ”representative” population) in the stellar population mix, while their metallicities were estimated from the CMD location of the most populous red giant branch track. The dispersion associated with the mean ages and metallicities result in general a satisfactory estimate of the age/metallicity spread, although some few individual representative subfields have slightly larger age/metallicity spread. As far as we are aware, these larger age spread do not affect the subsequent analysis. A detailed version of this work can be seen in Piatti et al. (2012, AJ, 144, 100). | - |
| dc.description | Fil: Piatti, Andres Eduardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Asociación Argentina de Astronomía | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/uploads/docs/baaa55.pdf | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.subject | galaxy | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Astrophysical properties of star fields in the Large Magellanic Cloud | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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