Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-24T03:36:59.172Z Has data issue: false hasContentIssue false
  • English
  • Français

Thermal and non thermal components of interstellar medium at sub-kiloparsec scales in galaxies

Published online by Cambridge University Press:  01 August 2006

Rosita Paladino
Rosita Paladino*
Affiliation:
INAF – Osservatorio Astronomico di Cagliari email: [email protected]
Rights & Permissions [Opens in a new window]

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.

We present the result of the analysis of the point-by-point correlation between the radio continuum (RC) and CO intensities from kpc to sub-kpc scales in 22 BIMA SONG galaxies and the point-by-point correlation at sub-kpc scales between the RC, CO and 24 μm-IR emissions in 6 galaxies for which Spitzer images have been recently released. We found that there is no significant variation of the slope and the scatter of the correlations at this spatial resolution. All three correlations are comparably tight with scatter of less than a factor of two.

Keywords

radio continuum: galaxiesgalaxies: spiralISM: moleculesstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 461
Copyright
Copyright © International Astronomical Union 2007

References

Paladino, R., Murgia, M., Helfer, T. T., Wong, T., Ekers, R., Blitz, L., Gregorini, L., & Moscadelli, L. 2006, A&A 456, 847Google Scholar