Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-11T11:29:34.376Z Has data issue: false hasContentIssue false
  • English
  • Français

Elemental abundance studies using the EBASIM spectrograph of the 2.1-m CASLEO Observatory telescope. I. The normal stars 5 Aqr and 30 Peg

Published online by Cambridge University Press:  02 March 2005

Saul J. Adelman ,
Zulema López-Garcia ,
Stella M. Malaroda ,
Natalia Núñez  and
Mónica Grosso
Saul J. Adelman
Affiliation:
Department of Physics, The Citadel, 171 Moultrie Street, Charleston, SC 29409, USA
Zulema López-Garcia
Affiliation:
Complejo Astronómico El Leoncito, Casilla de Correo 467, 5400 San Juan, Argentina Facultad de Ciencias Exactas, Físicas y Naturales, Universidad Nacional de San Juan, Cereseto y Meglioli, San Juan, Argentina Member of the Carrera del Investigador Cientifico, CONCIT, República Argentina
Stella M. Malaroda
Affiliation:
Complejo Astronómico El Leoncito, Casilla de Correo 467, 5400 San Juan, Argentina Facultad de Ciencias Exactas, Físicas y Naturales, Universidad Nacional de San Juan, Cereseto y Meglioli, San Juan, Argentina Member of the Carrera del Investigador Cientifico, CIC, República Argentina
Natalia Núñez
Affiliation:
Member of the Carrera del Investigador Cientifico, CONCIT, República Argentina
Mónica Grosso
Affiliation:
Complejo Astronómico El Leoncito, Casilla de Correo 467, 5400 San Juan, Argentina Facultad de Ciencias Exactas, Físicas y Naturales, Universidad Nacional de San Juan, Cereseto y Meglioli, San Juan, Argentina
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Using data from the new EBASIM spectrograph at the 2.1-m telescope of the Complejo Astronómico El Leoncito (CASLEO), two rather sharp-lined B stars 5 Aqr (=HD 198667, B9 III) and 30 Peg (=HD 211924, B5 IV) are being studied. The measurements are compared with those from the coudé spectrograph of the 1.22-m telescope of the Dominion Astrophysical Observatory (DAO). The equivalent width scales of the EBASIM and the DAO data are similar. As we found that the line profiles of 30 Peg are variable, we are trying to determine whether this star is a slowly pulsating B star. 5 Aqr has abundances close to those of the Sun.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Techniques: spectroscopicstars: abundancesstars: atmospheresstars: early-typestars: individual (5 Aqr, 30 Peg)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 530 - 532
Copyright
© 2004 International Astronomical Union