SDSS-IV MaNGA: Probing the Kinematic Morphology-Density Relation of Early-type Galaxies with MaNGA

J. E. Greene; A. Leauthaud; E. Emsellem; D. Goddard; J. Ge; B. H. Andrews; J. Brinkman; J. R. Brownstein; J. 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
, D. Goddard
, J. Ge
, B. H. Andrews
, J. Brinkman
, J. R. Brownstein
, J. 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

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

39 Scopus citations

Abstract

The kinematic morphologydensity 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 ^14.5 h^-1 M⊙ 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 (US)
Article number	L33
Journal	Astrophysical Journal Letters
Volume	851
Issue number	2
DOIs	https://doi.org/10.3847/2041-8213/aa8ace
State	Published - Dec 20 2017

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/2041-8213/aa8ace

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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., 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. Astrophysical Journal Letters, 851(2), Article L33. https://doi.org/10.3847/2041-8213/aa8ace

@article{148d98856bd34147a6802d5fd4a47291,

title = "SDSS-IV MaNGA: Probing the Kinematic Morphology-Density Relation of Early-type Galaxies with MaNGA",

abstract = "The kinematic morphologydensity 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 halo <10 14.5 h-1 M⊙ 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.",

author = "Greene, \{J. E.\} and A. Leauthaud and E. Emsellem and D. Goddard and J. Ge and Andrews, \{B. H.\} and J. Brinkman and Brownstein, \{J. R.\} and J. Greco 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",

note = "Funding Information: Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site iswww.sdss.org. Funding Information: J.E.G. is partially supported by NSF AST-1411642. We thank M. Cappellari for useful discussions. We thank the referee for constructive comments that improved this manuscript and we thank Ada Elizabeth Greene Silverman for waiting an extra week to come into this world while her mother submitted the initial manuscript.",

year = "2017",

month = dec,

day = "20",

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

language = "English (US)",

volume = "851",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

number = "2",

}

Greene, JE, Leauthaud, A, Emsellem, E, Goddard, D, Ge, J, Andrews, BH, Brinkman, J, Brownstein, JR, Greco, J, Law, D, Lin, YT, 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', Astrophysical Journal Letters, vol. 851, no. 2, L33. https://doi.org/10.3847/2041-8213/aa8ace

TY - JOUR

T1 - SDSS-IV MaNGA

T2 - Probing the Kinematic Morphology-Density Relation of Early-type Galaxies with MaNGA

AU - Greene, J. E.

AU - Leauthaud, A.

AU - Emsellem, E.

AU - Goddard, D.

AU - Ge, J.

AU - Andrews, B. H.

AU - Brinkman, J.

AU - Brownstein, J. R.

AU - Greco, J.

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.

N1 - Funding Information: Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site iswww.sdss.org. Funding Information: J.E.G. is partially supported by NSF AST-1411642. We thank M. Cappellari for useful discussions. We thank the referee for constructive comments that improved this manuscript and we thank Ada Elizabeth Greene Silverman for waiting an extra week to come into this world while her mother submitted the initial manuscript.

PY - 2017/12/20

Y1 - 2017/12/20

N2 - The kinematic morphologydensity 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 halo <10 14.5 h-1 M⊙ 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 morphologydensity 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 halo <10 14.5 h-1 M⊙ 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.

UR - https://www.scopus.com/pages/publications/85039744709

UR - https://www.scopus.com/pages/publications/85039744709#tab=citedBy

U2 - 10.3847/2041-8213/aa8ace

DO - 10.3847/2041-8213/aa8ace

M3 - Article

AN - SCOPUS:85039744709

SN - 2041-8205

VL - 851

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2

M1 - L33

ER -

SDSS-IV MaNGA: Probing the Kinematic Morphology-Density Relation of Early-type Galaxies with MaNGA

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