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Campo DC | Valor | Lengua/Idioma |
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dc.contributor.author | Román-Zúñiga, Carlos | - |
dc.contributor.author | Kounkel, Marina | - |
dc.contributor.author | Downes, José | - |
dc.date.accessioned | 2024-01-26T15:40:30Z | - |
dc.date.available | 2024-01-26T15:40:30Z | - |
dc.date.issued | 2023 | - |
dc.identifier.citation | Román-Zúñiga, C, Kounkel, M y Downes, J. "Stellar Properties for a Comprehensive Collection of Star-forming Regions in the SDSS APOGEE-2 Survey*". The Astronomical Journal. [en línea] 2023, 165(2): 51. 23 h. DOI: 10.3847/1538-3881/aca3a4 | es |
dc.identifier.issn | 1538-3881 | - |
dc.identifier.uri | https://hdl.handle.net/20.500.12008/42257 | - |
dc.description | Artículo escrito por 28 autores. | es |
dc.description.abstract | The Sloan Digital Sky Survey IV APOGEE-2 primary science goal was to observe red giant stars throughout the Galaxy to study its dynamics, morphology, and chemical evolution. The APOGEE instrument, a high-resolution 300-fiber H-band (1.55-1.71 μm) spectrograph, is also ideal to study other stellar populations in the Galaxy, among which are a number of star-forming regions and young open clusters. We present the results of the determination of six stellar properties (T eff, log g , [Fe/H], L/L ⊙, M/M ⊙, and age) for a sample that is composed of 3360 young stars, of subsolar to supersolar types, in 16 Galactic star formation and young open cluster regions. Those sources were selected by using a clustering method that removes most of the field contamination. Samples were also refined by removing targets affected by various systematic effects of the parameter determination. The final samples are presented in a comprehensive catalog that includes all six estimated parameters. This overview study also includes parameter spatial distribution maps for all regions and Hertzsprung-Russell ( log L / L ⊙ vs. T eff) diagrams. This study serves as a guide for detailed studies on individual regions and paves the way for the future studies on the global properties of stars in the pre-main-sequence phase of stellar evolution using more robust samples. | es |
dc.format.extent | 23 h. | es |
dc.format.mimetype | application/pdf | es |
dc.language.iso | en | es |
dc.publisher | American Astronomical Society | es |
dc.relation.ispartof | The Astronomical Journal, 2023, 165(2): 51 | es |
dc.rights | Las obras depositadas en el Repositorio se rigen por la Ordenanza de los Derechos de la Propiedad Intelectual de la Universidad de la República.(Res. Nº 91 de C.D.C. de 8/III/1994 – D.O. 7/IV/1994) y por la Ordenanza del Repositorio Abierto de la Universidad de la República (Res. Nº 16 de C.D.C. de 07/10/2014) | es |
dc.subject | Young star clusters | es |
dc.subject | Pre-main sequence stars | es |
dc.subject | Star forming regions | es |
dc.subject | Fundamental parameters of stars | es |
dc.subject | Near infrared astronomy | es |
dc.title | Stellar Properties for a Comprehensive Collection of Star-forming Regions in the SDSS APOGEE-2 Survey* | es |
dc.type | Artículo | es |
dc.contributor.filiacion | Román-Zúñiga Carlos | - |
dc.contributor.filiacion | Kounkel Marina | - |
dc.contributor.filiacion | Downes José, Universidad de la República (Uruguay). Facultad de Ciencias. Instituto de Física. | - |
dc.rights.licence | Licencia Creative Commons Atribución (CC - By 4.0) | es |
dc.identifier.doi | 10.3847/1538-3881/aca3a4 | - |
Aparece en las colecciones: | Publicaciones académicas y científicas - Facultad de Ciencias |
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10.3847.1538-3881.aca3a4 .pdf | 4,51 MB | Adobe PDF | Visualizar/Abrir |
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