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SDSS-IV MaNGA: signatures of halo assembly in kinematically misaligned galaxies

SDSS-IV MaNGA: signatures of halo assembly in kinematically misaligned galaxies
SDSS-IV MaNGA: signatures of halo assembly in kinematically misaligned galaxies
We investigate the relationship of kinematically misaligned galaxies with their large-scale environment, in the context of halo assembly bias. According to numerical simulations, halo age at fixed halo mass is intrinsically linked to the large-scale tidal environment created by the cosmic web. We investigate the relationship between distances to various cosmic web features and present-time gas accretion rate. We select a sub-sample of ∼900 central galaxies from the MaNGA survey with defined global position angles (PA; angle at which velocity change is greatest) for their stellar and H α gas components up to a minimum of 1.5 effective radii (Re). We split the sample by misalignment between the gas and stars as defined by the difference in their PA. For each central galaxy, we find its distance to nodes and filaments within the cosmic web, and estimate the host halo’s age using the central stellar mass to total halo mass ratio M*/Mh. We also construct halo occupation distributions using a background subtraction technique for galaxy groups split using the central galaxy’s kinematic misalignment. We find, at fixed halo mass, no statistical difference in these properties between our kinematically aligned and misaligned galaxies. We suggest that the lack of correlation could be indicative of cooling flows from the hot halo playing a far larger role than ‘cold mode’ accretion from the cosmic web or a demonstration that the spatial extent of current large-scale integral field unit surveys hold little information about large-scale environment extractable through this method.
1365-2966
172-188
Duckworth, Christopher
992c216c-8f66-48a8-8de6-2f04b4f736e6
Tojeiro, Rita
db934e1b-317a-4d86-8c2b-2ccdd75cd785
Kraljic, Katarina
44d870ee-8c7a-4149-bc04-d96b15fd9eeb
Sgró, Mario A
0f46b323-b0b2-463b-b39b-7236f2ff5cf4
Wild, Vivienne
0f7deb3d-3cdb-41b3-b39d-4184bae6d85d
Weijmans, Anne-Marie
eeef5841-558d-4553-81b8-6ae55c200657
Lacerna, Ivan
d26c2843-8490-4135-bb4e-d288a9ccb293
Drory, Niv
57bf18f8-de7a-4be9-94e2-88237a69d940
Duckworth, Christopher
992c216c-8f66-48a8-8de6-2f04b4f736e6
Tojeiro, Rita
db934e1b-317a-4d86-8c2b-2ccdd75cd785
Kraljic, Katarina
44d870ee-8c7a-4149-bc04-d96b15fd9eeb
Sgró, Mario A
0f46b323-b0b2-463b-b39b-7236f2ff5cf4
Wild, Vivienne
0f7deb3d-3cdb-41b3-b39d-4184bae6d85d
Weijmans, Anne-Marie
eeef5841-558d-4553-81b8-6ae55c200657
Lacerna, Ivan
d26c2843-8490-4135-bb4e-d288a9ccb293
Drory, Niv
57bf18f8-de7a-4be9-94e2-88237a69d940

Duckworth, Christopher, Tojeiro, Rita, Kraljic, Katarina, Sgró, Mario A, Wild, Vivienne, Weijmans, Anne-Marie, Lacerna, Ivan and Drory, Niv (2019) SDSS-IV MaNGA: signatures of halo assembly in kinematically misaligned galaxies. Monthly Notices Of The Royal Astronomical Society, 438 (1), 172-188. (doi:10.1093/mnras/sty3101).

Record type: Article

Abstract

We investigate the relationship of kinematically misaligned galaxies with their large-scale environment, in the context of halo assembly bias. According to numerical simulations, halo age at fixed halo mass is intrinsically linked to the large-scale tidal environment created by the cosmic web. We investigate the relationship between distances to various cosmic web features and present-time gas accretion rate. We select a sub-sample of ∼900 central galaxies from the MaNGA survey with defined global position angles (PA; angle at which velocity change is greatest) for their stellar and H α gas components up to a minimum of 1.5 effective radii (Re). We split the sample by misalignment between the gas and stars as defined by the difference in their PA. For each central galaxy, we find its distance to nodes and filaments within the cosmic web, and estimate the host halo’s age using the central stellar mass to total halo mass ratio M*/Mh. We also construct halo occupation distributions using a background subtraction technique for galaxy groups split using the central galaxy’s kinematic misalignment. We find, at fixed halo mass, no statistical difference in these properties between our kinematically aligned and misaligned galaxies. We suggest that the lack of correlation could be indicative of cooling flows from the hot halo playing a far larger role than ‘cold mode’ accretion from the cosmic web or a demonstration that the spatial extent of current large-scale integral field unit surveys hold little information about large-scale environment extractable through this method.

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More information

e-pub ahead of print date: 15 November 2018
Published date: 11 February 2019

Identifiers

Local EPrints ID: 472835
URI: http://eprints.soton.ac.uk/id/eprint/472835
ISSN: 1365-2966
PURE UUID: 56a7d0bb-9468-4d3d-9238-fcba1d8942a5
ORCID for Christopher Duckworth: ORCID iD orcid.org/0000-0003-0659-2177

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Date deposited: 20 Dec 2022 17:32
Last modified: 17 Mar 2024 04:06

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Contributors

Author: Christopher Duckworth ORCID iD
Author: Rita Tojeiro
Author: Katarina Kraljic
Author: Mario A Sgró
Author: Vivienne Wild
Author: Anne-Marie Weijmans
Author: Ivan Lacerna
Author: Niv Drory

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