Browsing by Author "Sankar, Sriram"

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    Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey
    (2023) Sankar, Sriram; Bershady, Matthew
    It is well known that galaxies shape and are shaped by their environments, but the relative contribution of environmental and internal galactic processes remains poorly understood. HI 21 cm is the ideal tracer to study the role of environments in shaping galaxies in the local universe as the extended distribution of neutral hydrogen makes it susceptible to a wide range of environmental effects that produce peculiar HI morphologies. Moreover, HI enables the study of how galaxies obtain and lose cold gas. The HI distribution of galaxies often exhibits warps, lopsidedness, and the presence of anomalous gas (AG) such as the Extraplanar Gas (EPG). In this era of resolved, sensitive HI observations, one exciting possibility is the identification of AG associated with galaxies experiencing a wide range of environmental effects. However, the task of separating AG and the disc is non-trivial due to fundamental limitations induced by instrumental effects (e.g., spatial and spectral resolution), projection effects, and systematic effects (e.g., assumptions, methods). In this work, we demonstrate a method we developed to separate anomalous gas from the disc based on physically motivated Gaussian decomposition and kinematic tagging. We perform a comprehensive analysis of the kinematics of the neutral gas in two nearby low-mass, gas-rich, late-type dominated, and relatively isolated groups from the MeerChoirs survey. The two groups, HIPASS J1250-20 and HIPASS J1403-06, both contain interacting pairs in the centre that showcase unique HI morphologies. In the groups, we investigate the impact of two ongoing co-rotating minor mergers, an intermediate-stage counter-rotating major merger, and an intermediate-stage co-rotating major merger. Additionally, we characterize several previously known and unknown dwarfs in the groups and the extended fields. We extract the kinematics of the extended, warped, and lopsided discs of the interacting galaxies using 3D tilted ring modelling. Employing techniques we developed, we detect and examine copious amounts of anomalous gas produced in the interactions in the form of leading gas, lagging gas, extended envelopes, tails, and bridges. By combining the kinematics, deep optical images, and ancillary evidence from the literature we relate the anomalous gas to star formation in the discs and the interactions. We detect gas exchange between the interacting pairs and enhanced star formation in the galaxies experiencing inflow. Notably, we report the farthest characterised EPG to date in HIPASS J1403:06 at a distance of 40 Mpc, which is also among the most massive EPG reservoirs ever studied. Furthermore, the 150 kpc long envelope of HIPASS J1250-20:S1 with a total HI mass of log MHI ∼ 10.72 M⊙ is among the most HI-rich galaxies in the literature. We posit plausible formation scenarios for the extended envelope in HIPASS J1250-20:S1 and the ∼ 90 kpc long unidirectional transverse tails observed in HIPASS J1403-06. We suspect misaligned gas accretion from companions for the former and a combination of collisional and tidal origin for the latter. Such studies of gas kinematics and galaxy dynamics across different environments will deepen our understanding of the baryon cycle, galaxy interactions, and the impact of the environment on galaxy evolution.
  • No Thumbnail Available
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    Open Access
    Kinematics of neutral hydrogen in interacting galaxies in two groups from the MeerChoirs survey
    (2023) Sankar, Sriram; Bershady, Matthew
    It is well known that galaxies shape and are shaped by their environments, but the relative contribution of environmental and internal galactic processes remains poorly understood. HI 21 cm is the ideal tracer to study the role of environments in shaping galaxies in the local universe as the extended distribution of neutral hydrogen makes it susceptible to a wide range of environmental effects that produce peculiar HI morphologies. Moreover, HI enables the study of how galaxies obtain and lose cold gas. The HI distribution of galaxies often exhibits warps, lopsidedness, and the presence of anomalous gas (AG) such as the Extraplanar Gas (EPG). In this era of resolved, sensitive HI observations, one exciting possibility is the identification of AG associated with galaxies experiencing a wide range of environmental effects. However, the task of separating AG and the disc is non-trivial due to fundamental limitations induced by instrumental effects (e.g., spatial and spectral resolution), projection effects, and systematic effects (e.g., assumptions, methods). In this work, we demonstrate a method we developed to separate anomalous gas from the disc based on physically motivated Gaussian decomposition and kinematic tagging. We perform a comprehensive analysis of the kinematics of the neutral gas in two nearby low-mass, gas-rich, late-type dominated, and relatively isolated groups from the MeerChoirs survey. The two groups, HIPASS J1250-20 and HIPASS J1403-06, both contain interacting pairs in the centre that showcase unique HI morphologies. In the groups, we investigate the impact of two ongoing co-rotating minor mergers, an intermediate-stage counter-rotating major merger, and an intermediate-stage co-rotating major merger. Additionally, we characterize several previously known and unknown dwarfs in the groups and the extended fields. We extract the kinematics of the extended, warped, and lopsided discs of the interacting galaxies using 3D tilted ring modelling. Employing techniques we developed, we detect and examine copious amounts of anomalous gas produced in the interactions in the form of leading gas, lagging gas, extended envelopes, tails, and bridges. By combining the kinematics, deep optical images, and ancillary evidence from the literature we relate the anomalous gas to star formation in the discs and the interactions. We detect gas exchange between the interacting pairs and enhanced star formation in the galaxies experiencing inflow. Notably, we report the farthest characterised EPG to date in HIPASS J1403:06 at a distance of 40 Mpc, which is also among the most massive EPG reservoirs ever studied. Furthermore, the 150 kpc long envelope of HIPASS J1250-20:S1 with a total HI mass of log MHI ∼ 10.72 M⊙ is among the most HI-rich galaxies in the literature. We posit plausible formation scenarios for the extended envelope in HIPASS J1250-20:S1 and the ∼ 90 kpc long unidirectional transverse tails observed in HIPASS J1403-06. We suspect misaligned gas accretion from companions for the former and a combination of collisional and tidal origin for the latter. Such studies of gas kinematics and galaxy dynamics across different environments will deepen our understanding of the baryon cycle, galaxy interactions, and the impact of the environment on galaxy evolution.