No CrossRef data available.
Article contents
Determining the Properties of Galaxy 2237+0305 using Gravitational Lensing
Published online by Cambridge University Press: 26 May 2016
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 have studied the mass distribution in the lensing galaxy 2237+0305 using constraints from both gravitational lensing and photometric and spectroscopic observations. We find that with sufficient dynamical information we can constrain the mass-to-light ratio of the luminous components and determine the dynamical contribution of the disk. in addition, future observations should allow us to place constraints on the shape of the dark matter halo and its inner slope.
- Type
- Part 4: Lensing
- Information
- Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 109 - 114
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
Huchra, J., Gorenstein, M., Kent, S., Shapiro, I., Smith, G., Horine, E. & Perley, R.
1985, AJ, 90, 691.CrossRefGoogle Scholar
Irwin, M., Webster, R., Hewett, P., Corrigan, R. & Jedrzejewski, R.
1989, AJ, 98, 1989.Google Scholar
Maller, A., Simard, L., Guhathakurta, P., Hjorth, J., Jaunsen, A., Flores, R. & Primack, J.
2000, ApJ, 533, 194.Google Scholar