Hostname: page-component-77c89778f8-sh8wx Total loading time: 0 Render date: 2024-07-18T11:16:07.438Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectrophotometry of Shell Galaxies

Published online by Cambridge University Press:  04 August 2017

W.D. Pence
W.D. Pence*
Affiliation:
The Space Telescope Science Institute, Homewood Campus, Baltimore, MD 21218

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.

Low dispersion spectra of two shell galaxies, NGC 3923 and NGC 3051, have been obtained covering the 5300Å to 10000Å spectral range. These long-slit spectra go through the nucleus of each galaxy and also through 12 shells in NGC 3923 and through 3 shells in NGC 3051. the main results are:

1) In NGC 3051 the surface brightness of the 2 inner shells is nearly constant with radius. These plateaus of luminosity have very abrupt outer cutoffs but have no detectable inner limits.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 463 - 464
Copyright
Copyright © Reidel 1987