Comparison of NIR and Hα emission from the HII regions of M100

Beckman, J. E.; Chan, S. J.
Bibliographical reference

Proceedings of the International Astronomical Union, Volume 292, pp. 327-327

Advertised on:
3
2013
Number of authors
2
IAC number of authors
1
Citations
1
Refereed citations
0
Description
We measure the flux values in the 4 Spitzer-IRAC bands, of a sample of 78 isolated luminous HII regions in the grand design galaxy M100. We estimate the near-IR luminosities and compare them with the Hα-luminosities from the Knapen HII-region catalogue. We find a strong, and expected positive correlation between the total IR luminosity and the Hα luminosity, but no significant correlation between the luminosity and the IR temperature of the regions.
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The basic objective of the broject is to investigate the evolution of galaxies by deepening our understanding of the interaction between the insterstellar medium and the stars.The main technique which we use is the two-dimensional kinematic study of whole galaxies observed using our instrument:GHaFaS, a Fabry-Perot interferometer on the William

Prof.
John E. Beckman