Extraplanar Emission-Line Gas in Edge-On Spiral Galaxies. II. Optical Spectroscopy

Details Extraplanar Emission-Line Gas in Edge-On Spiral Galaxies. II. Optical Spectroscopy Extraplanar Emission-Line Gas in Edge-On Spiral Galaxies. II. Optical Spectroscopy

2003-04-25

arxiv.org/abs/astro-ph/0304471v1

Astrophys.J. 592 (2003) 79-110

Astronomy and Astrophysics

Astrophysics

25 pages + several jpg figures. Accepted for publication in the Astrophysical Journal, Vol. 592, July 20 2003

Scientific paper

10.1086/375620

The results from deep long-slit spectroscopy of nine edge-on spiral galaxies with known extraplanar line emission are reported. Emission from Halpha, [N II] lambda 6548, 6583, and [S II] lambda 6716, 6731 is detected out to heights of a few kpc in all of these galaxies. Several other fainter diagnostic lines such as [O I] lambda 6300, [O III] lambda 4959, 5007, and He I lambda 5876 are also detected over a smaller scale. The relative strengths, centroids and widths of the various emission lines provide constraints on the electron density, temperature, reddening, source(s) of ionization, and kinematics of the extraplanar gas. In all but one galaxy, photoionization by massive OB stars alone has difficulties explaining all of the line ratios in the extraplanar gas. Hybrid models that combine photoionization by OB stars and another source of ionization such as photoionization by turbulent mixing layers or shocks provide a better fit to the data. The (upper limits on the) velocity gradients measured in these galaxies are consistent with the predictions of the galactic fountain model to within the accuracy of the measurements.

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