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Revista mexicana de astronomía y astrofísica

Print version ISSN 0185-1101

Rev. mex. astron. astrofis vol.40 n.2 Ciudad de México Oct. 2004

 

Line identification of the Si Star HD 87240

 

C. Saffe,1 H. Levato,2 and Z. López-García2

 

1 Observatorio Astronómico de Córdoba, Laprida 854, 5000, Córdoba, Argentina. On a fellowship from CONICET, Argentina. (sae@oac.uncor.edu).

2 Complejo Astronómico El Leoncito, C.C 467, 5400, San Juan, Argentina. Members of the Carrera del Investigador Científico, CONICET, Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina. (zlgarcia@casleo.gov.ar, hlevato@casleo.gov.ar).

 

Received 2004 August 2
Accepted 2004 September 17.

 

ABSTRACT

Line identifications are presented for the peculiar Ap Si star HD 87240(δ=–59° 51' 0.01") in the spectral region λλ3710–5520. This object is a member of the southern open cluster NGC 3114. Comparison of this object with other field silicon stars shows that it shares many of their line anomalies.

Key Words: Stars: Chemically Peculiar – Stars: Individual: HD 87240

 

RESUMEN

Se presentan las identificaciones de las líneas de la estrella peculiar tipo Ap Si HD 87240(δ=–59° 51' 0.01") en el intervalo espectral λλ3710–5520. Este objeto es miembro del cúmulo abierto meridional NGC 3114. La comparación de este objeto con otras estrellas Ap Si del campo muestra que tienen en común muchas de las anomalías en sus líneas.

 

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ACKNOWLEDGEMENTS

The present work was partially supported through a grant from the Consejo Nacional de Investigaciones Científicas y Tecnicas, República Argentina PIP 02147. ZLG acknowledges partial support by grants from the FONCYT, number 03-1505 and from CICITCA, UNSJ.

The authors acknowledge the use of the CCD and data reduction acquisition system at CASLEO.

 

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