SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA

J. E. Greene; A. Leauthaud; E. Emsellem; Daniel Goddard; J. Ge; B. H. Andrews; J. Brinkman; J. R. Brownstein; J. P. Greco; D. Law; Y. -T. Lin; K. L. Masters; M. Merrifield; S. More; N. Okabe; D. P. Schneider; D. Thomas; D. A. Wake; R. Yan; N. Drory

doi:10.3847/2041-8213/aa8ace

SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA

J. E. Greene
, A. Leauthaud
, E. Emsellem
, Daniel Goddard
, J. Ge
, B. H. Andrews
, J. Brinkman
, J. R. Brownstein
, J. P. Greco
, D. Law
, Y. -T. Lin
, K. L. Masters
, M. Merrifield
, S. More
, N. Okabe
, D. P. Schneider
, D. Thomas
, D. A. Wake
, R. Yan
, N. Drory

Institute of Cosmology & Gravitation

Research output: Contribution to journal › Article › peer-review

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Abstract

The "kinematic" morphology-density relation for early-type galaxies posits that those galaxies with low angular momentum are preferentially found in the highest-density regions of the universe. We use a large sample of galaxy groups with halo masses 10^12.5 < M_halo < 10^14.5h^-1 M_Θ observed with the Mapping Nearby Galaxies at APO (MaNGA) survey to examine whether there is a correlation between local environment and rotational support that is independent of stellar mass. We find no compelling evidence for a relationship between the angular momentum content of early-type galaxies and either local overdensity or radial position within the group at fixed stellar mass.

Original language	English
Article number	L33
Number of pages	6
Journal	The Astrophysical Journal
Volume	851
Issue number	2
DOIs	https://doi.org/10.3847/2041-8213/aa8ace
Publication status	Published - 13 Dec 2017

Keywords

astro-ph.GA
galaxies: elliptical and lenticular, cD
galaxies: groups: general
galaxies: kinematics and dynamics

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10.3847/2041-8213/aa8ace

1708.07843v1
Reproduced by permission of the AAS.
Accepted author manuscript (Post-print), 1.66 MB

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Greene, J. E., Leauthaud, A., Emsellem, E., Goddard, D., Ge, J., Andrews, B. H., Brinkman, J., Brownstein, J. R., Greco, J. P., Law, D., Lin, Y. .-T., Masters, K. L., Merrifield, M., More, S., Okabe, N., Schneider, D. P., Thomas, D., Wake, D. A., Yan, R., & Drory, N. (2017). SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA. The Astrophysical Journal, 851(2), Article L33. https://doi.org/10.3847/2041-8213/aa8ace

@article{c7f6fbf135fa40738fd78ff563bff788,

title = "SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA",

abstract = "The {"}kinematic{"} morphology-density relation for early-type galaxies posits that those galaxies with low angular momentum are preferentially found in the highest-density regions of the universe. We use a large sample of galaxy groups with halo masses 1012.5 < Mhalo < 1014.5h-1 MΘ observed with the Mapping Nearby Galaxies at APO (MaNGA) survey to examine whether there is a correlation between local environment and rotational support that is independent of stellar mass. We find no compelling evidence for a relationship between the angular momentum content of early-type galaxies and either local overdensity or radial position within the group at fixed stellar mass.",

keywords = "astro-ph.GA, galaxies: elliptical and lenticular, cD, galaxies: groups: general, galaxies: kinematics and dynamics",

author = "Greene, \{J. E.\} and A. Leauthaud and E. Emsellem and Daniel Goddard and J. Ge and Andrews, \{B. H.\} and J. Brinkman and Brownstein, \{J. R.\} and Greco, \{J. P.\} and D. Law and Lin, \{Y. -T.\} and Masters, \{K. L.\} and M. Merrifield and S. More and N. Okabe and Schneider, \{D. P.\} and D. Thomas and Wake, \{D. A.\} and R. Yan and N. Drory",

year = "2017",

month = dec,

day = "13",

doi = "10.3847/2041-8213/aa8ace",

language = "English",

volume = "851",

journal = "The Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2",

}

Greene, JE, Leauthaud, A, Emsellem, E, Goddard, D, Ge, J, Andrews, BH, Brinkman, J, Brownstein, JR, Greco, JP, Law, D, Lin, Y-T, Masters, KL, Merrifield, M, More, S, Okabe, N, Schneider, DP, Thomas, D, Wake, DA, Yan, R & Drory, N 2017, 'SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA', The Astrophysical Journal, vol. 851, no. 2, L33. https://doi.org/10.3847/2041-8213/aa8ace

TY - JOUR

T1 - SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA

AU - Greene, J. E.

AU - Leauthaud, A.

AU - Emsellem, E.

AU - Goddard, Daniel

AU - Ge, J.

AU - Andrews, B. H.

AU - Brinkman, J.

AU - Brownstein, J. R.

AU - Greco, J. P.

AU - Law, D.

AU - Lin, Y. -T.

AU - Masters, K. L.

AU - Merrifield, M.

AU - More, S.

AU - Okabe, N.

AU - Schneider, D. P.

AU - Thomas, D.

AU - Wake, D. A.

AU - Yan, R.

AU - Drory, N.

PY - 2017/12/13

Y1 - 2017/12/13

N2 - The "kinematic" morphology-density relation for early-type galaxies posits that those galaxies with low angular momentum are preferentially found in the highest-density regions of the universe. We use a large sample of galaxy groups with halo masses 1012.5 < Mhalo < 1014.5h-1 MΘ observed with the Mapping Nearby Galaxies at APO (MaNGA) survey to examine whether there is a correlation between local environment and rotational support that is independent of stellar mass. We find no compelling evidence for a relationship between the angular momentum content of early-type galaxies and either local overdensity or radial position within the group at fixed stellar mass.

AB - The "kinematic" morphology-density relation for early-type galaxies posits that those galaxies with low angular momentum are preferentially found in the highest-density regions of the universe. We use a large sample of galaxy groups with halo masses 1012.5 < Mhalo < 1014.5h-1 MΘ observed with the Mapping Nearby Galaxies at APO (MaNGA) survey to examine whether there is a correlation between local environment and rotational support that is independent of stellar mass. We find no compelling evidence for a relationship between the angular momentum content of early-type galaxies and either local overdensity or radial position within the group at fixed stellar mass.

KW - astro-ph.GA

KW - galaxies: elliptical and lenticular, cD

KW - galaxies: groups: general

KW - galaxies: kinematics and dynamics

U2 - 10.3847/2041-8213/aa8ace

DO - 10.3847/2041-8213/aa8ace

M3 - Article

SN - 0004-637X

VL - 851

JO - The Astrophysical Journal

JF - The Astrophysical Journal

IS - 2

M1 - L33

ER -

SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA

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Keywords

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