Luminosity-colour relations for red clump stars

Bibcode
2013Ap&SS.344..417B
DOI
10.1007/s10509-012-1342-9
Çakmak, H.; Cabrera-Lavers, A.; Karaali, S.; Önal, Ö.; Bilir, S.
Referencia bibliográfica

Astrophysics and Space Science, Volume 344, Issue 2, pp.417-427

Fecha de publicación:
4
2013
Revista
Astrophysics and Space Science
Número de autores
5
Número de autores del IAC
1
Número de citas
12
Número de citas referidas
12
Descripción
We calibrated the absolute magnitudes M V , M J , M_{Ks} and M g of red clump stars in terms of colours. M V and M g are strongly dependent on colour, while the dependence of M J and M_{Ks} on colour is rather weak. The calibration of the absolute magnitudes M V and M_{Ks} is tested on 101 RC stars in the field SA 141. The Galactic model parameters estimated with this sample are in good agreement with earlier studies.
Proyectos relacionados
Project Image
Morfología y dinámica de la Vía Láctea
El Proyecto se estructura en dos partes, diferenciadas pero complementarias: morfología y dinámica. El estudio detallado de la morfología de la Vía Láctea pretende proveer una base de datos de distribución estelar en las regiones más alejadas y extintas de nuestra Galaxia, mediante el desarrollo de modelos semiempíricos a partir de la información
Martín
López Corredoira
En ejecución
Tipo
Con árbitro
La Vía Láctea y el Grupo Local (MWLG)

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