Bibcode
Zamora, O.; Abia, C.; de Laverny, P.; Domínguez, I.
Referencia bibliográfica
Memorie della Società Astronomica Italiana, v.75, p.596 (2004)
Fecha de publicación:
0
2004
Número de citas
1
Número de citas referidas
1
Descripción
We discuss the use of the spectral range near 7570 Å to determine
the Mg isotopic ratios in carbon stars using the
B'2 Sigma +-X 2 Sigma
+ system of the MgH molecule. We also compare with the
spectral range near 5140 Å that has been commonly used in normal
stars (oxygen-rich stars). The region near 5140 Å is not the
better choice for carbon stars because it is very crowded with CN and
C_2 molecular bands and the localization of the continuum is
complicated. The range near 7570 Å is less blended with molecular
bands. The continuum is easy to locate and the isotopic splitting
between MgH isotopic absorptions is larger. Unfortunately, we are not
able to reproduce accurately the observed spectrum in this region and,
moreover, the synthetic spectrum is not sensitive to large variations in
the isotopic ratios.