Hostname: page-component-77c89778f8-gvh9x Total loading time: 0 Render date: 2024-07-16T17:51:44.211Z Has data issue: false hasContentIssue false
  • English
  • Français

Ultraviolet Energy Distributions of (32) Early–Type Galaxies

Published online by Cambridge University Press:  04 August 2017

F. Bertola ,
D. Burstein ,
L.M. Buson ,
S.M. Faber  and
T.R. Lauer
F. Bertola
Affiliation:
Institute of Astronomy, University of Padova, Italy
D. Burstein
Affiliation:
Arizona State University, Tempe, USA
L.M. Buson
Affiliation:
Astronomical Observatory, Padova, Italy
S.M. Faber
Affiliation:
University of California, Santa Cruz, USA
T.R. Lauer
Affiliation:
Princeton University, Princeton, USA

Extract

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.

New, self–consistent energy distribution have been generated from 52 short – wavelength and 40 long–wavelength IUE spectra of 31 early–type galaxies, plus the bulge of M31. All galaxies in this sample have measurements of the absorption–line index Mg2 and central velocity dispersion, and a (1550–V) color is determined by combing the IUE data with photoelectrically–measured V magnitudes.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 439
Copyright
Copyright © Reidel 1987