The Halogas Project: HI Observations Of NGC 1003

Astronomy and Astrophysics – Astronomy

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Scientific paper

We present deep neutral hydrogen observations of the nearby spiral galaxy NGC 1003, obtained as part of the Westerbork Hydrogen Accretion in LOcal GAlaxieS (HALOGAS) Survey currently being performed with the Westerbork Synthesis Radio Telescope (WSRT). Our data are sensitive enough to detect and study both faint diffuse neutral hydrogen gas, as well as discrete accreting gas clouds. We have performed careful tilted-ring modeling of NGC 1003, which shows that it is nearly edge-on, and has a significant warp. The HI disk is both thick (scale height 1 kpc) and radially extended (4-5 times larger than the optical disk). We also present the results of our analysis of the extraplanar gas cloud population in this galaxy. We detect two discrete clouds in the halo of NGC 1003, both with HI masses of about two hundred thousand solar masses, and a larger extraplanar gas complex with an HI mass of about two million solar masses. These extraplanar gas features are analogous to high- and intermediate-velocity clouds around the Milky Way. We discuss the implications of these features for the accretion history of NGC 1003.

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