Optical observations of the nearby galaxy NGC 2366 through narrowband H and SII filters. Supernova remnants status
arXiv:1902.08671 · doi:10.2298/SAJ190131003V
Abstract
We present detection of 67 HII regions and two optical supernova remnant (SNR) candidates in the nearby irregular galaxy NGC 2366. The SNR candidates were detected by applying [SII]/H ratio criterion to observations made with the 2-m RCC telescope at Rozhen National Astronomical Observatory in Bulgaria. In this paper we report coordinates, diameters, H and [SII] fluxes for detected objects across the two fields of view in NGC 2366 galaxy. Using archival XMM-Newton observations we suggest possible X-ray counterparts of two optical SNR candidates. Also, we discard classification of two previous radio SNR candidates in this galaxy, since they appear to be background galaxies.
12 pages, 6 figures, accepted for publication in Serbian Astronomical Journal