Accession Number : ADA483744


Title :   Enormous Disc of Cool Gas Surrounding the Nearby Powerful Radio Galaxy NGC 612 (PKS 0131-36)


Descriptive Note : Journal article


Corporate Author : COLUMBIA UNIV NEW YORK DEPT OF ASTRONOMY


Personal Author(s) : Emonts, B H ; Morganti, R ; Oosterloo, T A ; Holt, J ; Tadhunter, C N ; Hulst, van der, J M ; Ojha, R ; Sadler, E M


Full Text : https://apps.dtic.mil/dtic/tr/fulltext/u2/a483744.pdf


Report Date : 22 May 2008


Pagination or Media Count : 15


Abstract : We present the detection of an enormous disc of cool neutral hydrogen (HI) gas surrounding the SO galaxy NGC 612, which hosts one of the nearest powerful radio sources (PKS 0131-36). Using the Australia Telescope Compact Array, we detect M(HI) = 1.8 x 10(9) M(.) of HI emission-line gas that is distributed in a 140 kpc wide disc-like structure along the optical disc and dust-lane of NGC 612. The bulk of the gas in the disc appears to be settled in regular rotation with a total velocity range of 850 km s(-1), although asymmetries in this disc indicate that perturbations are being exerted on part of the gas, possibly by a number of nearby companions. The HI disc in NGC 612 suggests that the total mass enclosed by the system is M(enc) 2.9 x 10(12) sin (-2i) M(.), implying that this early-type galaxy contains a massive dark matter halo. We also discuss an earlier study by Holt et al. that revealed the presence of a prominent young stellar population at various locations throughout the disc of NGC 612, indicating that this is a rare example of an extended ratio source that is hosted by a galaxy with a large-scale star-forming disc. In addition, we map a faint HI bridge along a distance of 400 kpc in between NGC 612 and gas-rich (M(HI) = 8.9 x 10(9) M(.)) barred galaxy NGC 619, indicating that likely an interaction between both systems occurred. From the unusual amounts of HI gas and young stars in this early-type galaxy, in combination with the detection of a faint optical shell and the system's high infra-red luminosity, we argue that either ongoing or past galaxy interactions or a major merger event are a likely mechanism for the triggering of the radio source in NGC 612. This paper is part of an ongoing study to map the large-scale neutral hydrogen properties of nearby radio galaxies and it presents the first example of large-scale HI detected around a powerful Fanaroff & Riley type-II (FR-II) radio galaxy.


Descriptors :   *HYDROGEN , *GALAXIES , INFRARED PHENOMENA , REPRINTS , KINEMATICS


Subject Categories : Meteorology


Distribution Statement : APPROVED FOR PUBLIC RELEASE