No CrossRef data available.
Article contents
Gas kinematics and stellar archaeology of the Seyfert galaxy NGC 5643
Published online by Cambridge University Press: 29 March 2021
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.
In this work we derive stellar archaeology and kinematics of the central 400 pc of NGC 5643. The star formation history (SFH) reveals nuclear contribution of stellar populations older (20% older than 3.5 Gyr) and younger (60% younger than 320 Myr) as compared to the circumnuclear region. The [OIII] 5007 Å kinematics reveals the eastern ionization cone with an outflow (−60 km/s ⩽ v ⩽ 120 km/s).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 452 - 453
- Copyright
- © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union
References
Cid Fernandes, R., Mateus, A., Sodré, L., et al. 2005, MNRAS, 350, 363
10.1111/j.1365-2966.2005.08752.xCrossRefGoogle Scholar
Schmitt, H. R., Storchi-Bergmann, T., Baldwin, J. A., et al. 1994, ApJ, 423, 237
10.1086/173802CrossRefGoogle Scholar
Simpson, C., Wilson, A. S., Bower, G., et al. 1997, ApJ 474, 121
10.1086/303466CrossRefGoogle Scholar
You have
Access