New fundamental parameters for the inner disk open cluster Lyngå 11
We have obtained CCD BVIKC photometry down to V ∼ 21.5 for the open cluster Lyngå 11 and its surrounding field. This previously unstudied object appears to be rich and highly absorbed. A cluster angular radius of 4.5′ ± 0.5′, equivalent to (3.0 ± 0.3) pc, is estimated from star counts in 100-pixel a...
Guardado en:
Publicado: |
2006
|
---|---|
Materias: | |
Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_13841076_v11_n4_p262_Piatti http://hdl.handle.net/20.500.12110/paper_13841076_v11_n4_p262_Piatti |
Aporte de: |
Ejemplares similares
-
New fundamental parameters for the inner disk open cluster Lyngå 11
por: Piatti, A.E., et al. -
NGC 2587: A sparse open cluster projected on to a populous star field
Publicado: (2009) -
NGC 2587: A sparse open cluster projected on to a populous star field
por: Piatti, A.E., et al. -
Improvements on the fundamental parameters of the open cluster Tombaugh 1 through Washington system photometry
Publicado: (2004) -
Improvements on the fundamental parameters of the open cluster Tombaugh 1 through Washington system photometry
por: Piatti, A.E., et al.