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

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SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA. / Greene, J. E.; Leauthaud, A.; Emsellem, E.; Goddard, Daniel; 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.

In: The Astrophysical Journal, Vol. 851, No. 2, L33, 13.12.2017.

Research output: Contribution to journalArticle

Harvard

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

APA

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), [L33]. https://doi.org/10.3847/2041-8213/aa8ace

Vancouver

Greene JE, Leauthaud A, Emsellem E, Goddard D, Ge J, Andrews BH et al. SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA. The Astrophysical Journal. 2017 Dec 13;851(2). L33. https://doi.org/10.3847/2041-8213/aa8ace

Author

Greene, J. E. ; Leauthaud, A. ; Emsellem, E. ; Goddard, Daniel ; 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. / SDSS-IV MaNGA: probing the kinematic morphology-density relation of early-type galaxies with MaNGA. In: The Astrophysical Journal. 2017 ; Vol. 851, No. 2.

Bibtex

@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 = "IOP Publishing",
number = "2",

}

RIS

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

VL - 851

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - L33

ER -

ID: 7714329