Molecular gas kinematics and line diagnostics in early-type galaxies: NGC 4710 & NGC 5866

Topal, Selçuk, Bureau, Martin, Davis, Timothy A. ORCID: https://orcid.org/0000-0003-4932-9379, Krips, Melanie, Young, Lisa M. and Crocker, Alison F. 2016. Molecular gas kinematics and line diagnostics in early-type galaxies: NGC 4710 & NGC 5866. Monthly Notices of the Royal Astronomical Society 463 (4) , pp. 4121-4152. 10.1093/mnras/stw2257

Preview

PDF - Accepted Post-Print Version Download (7MB) | Preview

Abstract

We present interferometric observations of CO lines (12CO(1-0, 2-1) and 13CO(1-0, 2-1)) and dense gas tracers (HCN(1-0), HCO+(1-0), HNC(1-0) and HNCO(4-3)) in two nearby edge-on barred lenticular galaxies, NGC 4710 and NGC 5866, with most of the gas concentrated in a nuclear disc and an inner ring in each galaxy. We probe the physical conditions of a two-component molecular interstellar medium in each galaxy and each kinematic component by using molecular line ratio diagnostics in three complementary ways. First, we measure the ratios of the position-velocity diagrams of different lines, second we measure the ratios of each kinematic component's integrated line intensities as a function of projected position, and third we model these line ratios using a non-local thermodynamic equilibrium radiative transfer code. Overall, the nuclear discs appear to have a tenuous molecular gas component that is hotter, optically thinner and with a larger dense gas fraction than that in the inner rings, suggesting more dense clumps immersed in a hotter more diffuse molecular medium. This is consistent with evidence that the physical conditions in the nuclear discs are similar to those in photo-dissociation regions. A similar picture emerges when comparing the observed molecular line ratios with those of other galaxy types. The physical conditions of the molecular gas in the nuclear discs of NGC 4710 and NGC 5866 thus appear intermediate between those of spiral galaxies and starbursts, while the star formation in their inner rings is even milder

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Publisher:	Oxford University Press
ISSN:	0035-8711
Funders:	STFC
Date of First Compliant Deposit:	22 September 2016
Date of Acceptance:	6 September 2016
Last Modified:	16 Nov 2024 07:30
URI:	https://orca.cardiff.ac.uk/id/eprint/94553

Citation Data

Cited 6 times in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item