Abstract Details
| Name: Narendra Nath Patra Affiliation: NCRA-TIFR Conference ID: ASI2015_602 Title : Modeling HI distribution and kinematics in the edge-on dwarf irregular galaxy KK250 Authors and Co-Authors : Arunima Banerjee(IUCAA) Jayaram N Chengalur (NCRA) Ayesha Begum Sinha (IISER, Bhopal) Abstract Type : Oral Abstract Category : Extragalactic astronomy Abstract : We model the observed vertical distribution of the neutral hydrogen (HI) in the faint (M$_{\rm B} \sim -13.7$~mag) edge-on dwarf irregular galaxy KK250. Our model assumes that the galaxy consists of axi-symmetric, co-planar gas and stellar discs in the external force-field of a spherical dark matter halo, and in vertical hydrostatic equilibrium. The velocity dispersion of the gas is left as a free parameter in the model. Our best fit model is able to reproduce the observed vertical distribution of the HI gas, as well as the observed velocity profiles. The best fit model has a large velocity dispersion ($\sim 22$~\kms) at the centre of the galaxy, which falls to a value of $\sim 8$~\kms\ by a galacto-centric radius of 1 kpc, which is similar to both the scale-length of the stellar disc, as well as the angular resolution of the data along the radial direction. Similarly we find that the thickness of the HI disc is also minimum at $\sim 1$kpc, and increases by about a factor of $\sim 2$ as one goes to the centre of the galaxy or out to $\sim 3$kpc. The minimum intrinsic HWHM of the HI vertical distribution in KK250 is $\sim 350$pc. For comparison the HWHM of the vertical distribution of the HI in the solar neighbourhood is $\sim 70-140$~pc. Our results are hence consistent with other observations which indicate that dwarf galaxies have significantly puffier gas discs than spirals. |