Hostname: page-component-7c8c6479df-5xszh Total loading time: 0 Render date: 2024-03-28T12:33:22.940Z Has data issue: false hasContentIssue false

Radial distributions of spectral absorption indices in spiral disks

Published online by Cambridge University Press:  01 December 2006

Mercedes Mollá*
Affiliation:
CIEMAT, Avda. Complutense 22, 28040 Madrid (Spain) email: mercedes.molla@ciemat.es
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.

We present a grid of 440 spectro-photometric models for simulating spiral and irregular galaxies. They have been consistently calculated with evolutionary synthesis models which use as input the information proceeding from chemical evolution models. The model predictions are spectral energy distributions, brightness and color profiles and radial distributions of spectral absorption stellar indices which are in agreement with observations

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Beauchamp, D., & Hardy, E. 1997, AJ, 113, 1666CrossRefGoogle Scholar
Cantin, S., Robert, C., Pellerin, A. & Mollá, M. 2005, New Astronomy Review, 49, 536CrossRefGoogle Scholar
Mollá, M., & Díaz, A. I. 2005, MNRAS, 358, 521CrossRefGoogle Scholar
Mollá, M., Hardy, E., & Beauchamp, D. 1999, ApJ, 513, 695CrossRefGoogle Scholar
Ryder, S. D., Fenner, Y., & Gibson, B. K. 2005, MNRAS, 358, 1337CrossRefGoogle Scholar
Warmels, R. H. 1988, A&AS, 72, 427Google Scholar