Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-27T13:03:47.951Z Has data issue: false hasContentIssue false
  • English
  • Français

IR imaging of spiral galaxy bulges

Published online by Cambridge University Press:  07 August 2017

Dennis Zaritsky ,
Marcia Rieke  and
Hans-Walter Rix
Dennis Zaritsky
Affiliation:
Carnegie Observatories, 813 Santa Barbara St., Pasadena, CA, 91101, U.S.A.
Marcia Rieke
Affiliation:
Steward Observatory, Univ. of Arizona, Tucson, AZ, 85721, U.S.A.
Hans-Walter Rix
Affiliation:
Institute for Advanced Study, Princeton, NJ, 08540, U.S.A.

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.

Imaging in the infrared (2.2μ) minimizes the impact of dust obscuration and allows reliable mapping of the mass-tracing stellar population in spiral galaxies. We find dramatic differences compared to photometry at shorter wavelengths (e.g. 0.8μ). As an example, the observations of the mini-bar and inner spiral arms of M 51 are discussed.

Keywords

galaxies: photometrygalaxies: spiralgalaxies: individual: M 51
Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 441 - 442
Copyright
Copyright © Kluwer 1993 

References

Binney, J. and Tremaine, S. (1987), Galactic Dynamics, (Princeton University Press: Princeton).Google Scholar
Goad, J.W., DeVeny, J.B., and Goad, L.E. (1979), Ap. J. Suppl., 39, 439.Google Scholar
Hernquist, L. (1990), in Dynamics and Interactions of Galaxies, ed. Wielen, R., (Heidelberg: Springer-Verlag), p. 108.Google Scholar
Pierce, M.J. (1986), A.J., 92, 285.Google Scholar
Tully, R.B. (1974), Ap. J. Suppl., 27, 449.Google Scholar
Zaritsky, D., and Lo, K.-Y. (1986), Ap. J., 303, 66.Google Scholar