Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-23T11:57:39.266Z Has data issue: false hasContentIssue false
  • English
  • Français

High resolution infrared maps of IRAS galaxies

Published online by Cambridge University Press:  03 August 2017

S. K. Ghosh ,
T. N. Rengarajan  and
R. P. Verma
S. K. Ghosh
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, Bombay 400 005, India
T. N. Rengarajan
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, Bombay 400 005, India
R. P. Verma
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, Bombay 400 005, India

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.

IRAS has provided infrared maps of a large number of galaxies. However the size of IRAS survey detectors is quite large (∼5′ in the cross-scan direction) and there is a need for improving the resolution of these maps. In order to understand the spatial structure of galaxies, we have generated high resolution maps of 18 large galaxies by deconvolving the IRAS pointed observations from survey detectors as well as from Chopped Photometric Channel (CPC) using Maximum Entropy Method (MEM).

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 411 - 412
Copyright
Copyright © Kluwer 1991