No CrossRef data available.
Article contents
The Stellar Content in the Central Region of M81
Published online by Cambridge University Press: 25 May 2016
Abstract
Using long slit spectroscopy, we investigate the stellar population and reddening gradients inside the central regions of the nearby spiral galaxy M81. Observational data are analyzed using a new mathematical method. The basic elements to construct the synthetic spectra are taken from a database of star spectra. We show the ability of this method to define detailed stellar populations and to differentiate between age and metallicity effects.
- Type
- Part 3: Star Formation Processes and Chemical Evolution
- Information
- Symposium - International Astronomical Union , Volume 192: The Stellar Content of Local Group Galaxies , 1999 , pp. 373 - 376
- Copyright
- Copyright © Astronomical Society of the Pacific 1999