Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-09-24
Mon.Not.Roy.Astron.Soc. 329 (2002) 481
Astronomy and Astrophysics
Astrophysics
Accepted for publication in MNRAS, large figures available on a separate tarfile
Scientific paper
10.1046/j.1365-8711.2002.04967.x
We have obtained accurate CCD narrow band H_beta and H_alpha photometry of Giant HII Regions in M 33, NGC 6822 and M 101. Comparison with previous determinations of emission line fluxes show large discrepancies; their probable origins are discussed. Combining our new photometric data with global velocity dispersion (sigma) derived from emission line widths we have reviewed the L(H_beta)-sigma relation. A reanalysis of the properties of the GEHRs included in our sample shows that age spread and the superposition of components in multiple regions introduce a considerable spread in the regression. Combining the information available in the literature regarding ages of the associated clusters, evolutionary footprints on the interstellar medium, and kinematical properties of the knots that build up the multiple GEHRs, we have found that a subsample - which we refer to as young and single GEHRs - do follow a tight relation in the L-sigma plane.
Bosch Guillermo L.
Terlevich Elena
Terlevich Robert
No associations
LandOfFree
Narrowband CCD Photometry of Giant HII Regions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Narrowband CCD Photometry of Giant HII Regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Narrowband CCD Photometry of Giant HII Regions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-307663