Deep Fabry-Perot Halpha observations of two Sculptor group galaxies, NGC 247 and NGC 300

TL;DR

This study used deep Halpha Fabry-Perot observations to analyze the distribution of ionized gas in two Sculptor group galaxies, NGC 247 and NGC 300, revealing details about their gas extent and implications for dark matter distribution.

Contribution

It provides the deepest Halpha observations of these galaxies, extending optical rotation curves and analyzing the presence of diffuse ionized gas relative to HI discs and galaxy warps.

Findings

NGC 247 shows Halpha emission up to its HI disc but not beyond.

NGC 300 has ionized gas detected throughout the observed field.

Results suggest ionization is linked to galaxy warps and star formation activity.

Abstract

It has been suggested that diffuse ionized gas can extend all the way to the end of the HI disc, and even beyond, such as in the case of the warped galaxy NGC 253 (Bland-Hawthorn et al. 1997). Detecting ionized gas at these radii could carry significant implications as to the distribution of dark matter in galaxies. With the aim of detecting this gas, we carried out a deep Halpha kinematical analysis of two Sculptor group galaxies, NGC 247 and NGC 300. The Fabry-Perot data were taken at the 36-cm Marseille Telescope in La Silla, Chile, offering a large field of view. With almost 20 hours of observations for each galaxy, very faint diffuse emission is detected. Typical emission measures of 0.1 cm^-6 pc are reached. For NGC 247, emission extending up to a radius comparable with that of the HI disc (r~13') is found, but no emission is seen beyond the HI disc. For NGC 300, we detect ionized gas on the entirety of our field of view (r_max~14'), and find that the bright HII regions are embedded in a diffuse background. Using the deep data, extended optical rotation curves are obtained, as well as mass models. These are the most extended optical rotation curves thus far for these galaxies. We find no evidence suggesting that NGC 247 has a warped disc, and to account for our non detection of Halpha emission beyond its HI disc, as opposed to the warped galaxy NGC 253, our results favour the model in which only through a warp, ionization by hot young stars in the central region of a galaxy can let photons escape and ionize the interstellar medium in the outer parts.