Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-24T02:22:01.797Z Has data issue: false hasContentIssue false
  • English
  • Français

U-G and G-R Colors of the Clumpy Irregular Galaxies Markarian 297 and 325

Published online by Cambridge University Press:  04 August 2017

S. Tamura  and
J. Heidmann
S. Tamura
Affiliation:
Astronomical Institute, Tohuko University, Sendai 980, Japan
J. Heidmann
Affiliation:
Observatoire de Paris, 92125 Meudon, France

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.

U-G and G-R colors of clumps in Mrk 297 and Mrk 325 are presented. In addition, colors of other interesting objects and radiation sources were calculated for the Kiso UGR system. These objects are used to interpret the intrinsic characteristics of our sample. The observed colors of the clumps in both Mrk 297 and Mrk 325 are bluer than Im galaxies as well as main sequence stars and show scatter over the extent of the U-G vs. G-R diagram.

Type
II. Large Scale Processes of Star Formation
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 642 - 644
Copyright
Copyright © Reidel 1987