Magnesium-to-Iron Ratio in Nuclei and Bulges of Disk Galaxies

Details Magnesium-to-Iron Ratio in Nuclei and Bulges of Disk Galaxies Magnesium-to-Iron Ratio in Nuclei and Bulges of Disk Galaxies

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ap%26ss.265..389s&link_type=abstract

Astrophysics and Space Science, v. 265, Issue 1/4, p. 389-390 (1999).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The results of magnesium-to-iron ratio estimates are presented for the nuclei and central bulges of disk galaxies. A great variety of behaviours is found: the nuclei have solar Mg/Fe ratio or are Mg-overabundant, the bulges can be more or less Mg-overabundant than the nuclei. But the most bulges have nearly solar Mg/Fe ratios, irrespective of their luminosity.

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