C.D.S. - SIMBAD4 rel 1.7 - 2020.07.12CEST15:25:09

1998A&A...338...15R - Astronomy and Astrophysics, volume 338, 15-26 (1998/10-1)

Internal turbulence, viriality, and density bounding of the most luminous HII regions in the spiral galaxy M 100.


Abstract (from CDS):

We present TAURUS Fabry-Perot velocity data in Hα emission of the disc of the grand design spiral M 100 (NGC 4321). We have studied the emission spectra of the 200 HII regions most luminous in Hα, calibrated in luminosity using photometric Hα imaging from the literature. The emission spectra of individual HII regions were fitted using one or more Gaussian functions, and analyzed in terms of their velocity dispersion. We concentrate on the question of whether the emission lines show values of their internal velocity dispersions of HII regions which would be predicted from the virial theorem, and find that in general this is not the case. There is a systematic trend to super-virial line widths, characteristic of the non-equilibrium effects of powerful OB stellar winds, and supernovae. We propose that the lower envelope in velocity dispersion σ, in the plot of Hα luminosity v. σ represents the virialized regions, and give a tentative theoretical explanation for its slope of 2.6 in the log-log plane, in terms of density bounding for the regions of highest luminosity.

Abstract Copyright:

Journal keyword(s): ISM: HII regions - galaxies: individual: M100 - galaxies: spiral - galaxies: structure - galaxies: ISM

Simbad objects: 3

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Number of rows : 3

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
1 M 33 GiG 01 33 50.904 +30 39 35.79 6.17 6.27 5.72     ~ 5135 1
2 NGC 604 HII 01 34 32.1 +30 47 01           ~ 544 0
3 M 100 AGN 12 22 54.9318850854 +15 49 20.294302163 10.04 10.05 9.35     ~ 1647 2

    Equat.    Gal    SGal    Ecl

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