Skip to main content

  2. Astrophysical Sciences

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

Author(s): Greene, Jenny E.; Leauthaud, A; Emsellem, E; Goddard, D; Ge, J; et al

Download
To refer to this page use: http://arks.princeton.edu/ark:/88435/pr17731
Full metadata record
DC FieldValueLanguage
dc.contributor.authorGreene, Jenny E.-
dc.contributor.authorLeauthaud, A-
dc.contributor.authorEmsellem, E-
dc.contributor.authorGoddard, D-
dc.contributor.authorGe, J-
dc.contributor.authorAndrews, BH-
dc.contributor.authorBrinkman, J-
dc.contributor.authorBrownstein, JR-
dc.contributor.authorGreco, J-
dc.contributor.authorLaw, D-
dc.contributor.authorLin, Y-T-
dc.contributor.authorMasters, KL-
dc.contributor.authorMerrifield, M-
dc.contributor.authorMore, S-
dc.contributor.authorOkabe, N-
dc.contributor.authorSchneider, DP-
dc.contributor.authorThomas, D-
dc.contributor.authorWake, DA-
dc.contributor.authorYan, R-
dc.contributor.authorDrory, N-
dc.date.accessioned2019-08-29T17:04:22Z-
dc.date.available2019-08-29T17:04:22Z-
dc.date.issued2017-12-20en_US
dc.identifier.citationGreene, JE, Leauthaud, A, Emsellem, E, Goddard, D, Ge, J, Andrews, BH, Brinkman, J, Brownstein, JR, Greco, J, 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. ASTROPHYSICAL JOURNAL LETTERS, 851 (10.3847/2041-8213/aa8aceen_US
dc.identifier.issn2041-8205-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr17731-
dc.description.abstractThe “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(14.5) h(-1) M-circle dot 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.en_US
dc.language.isoen_USen_US
dc.relationhttp://simbad.u-strasbg.fr/simbad/sim-ref?querymethod=bib&simbo=on&submit=submit+bibcode&bibcode=2017ApJ...851L..33Gen_US
dc.relation.ispartofASTROPHYSICAL JOURNAL LETTERSen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleSDSS-IV MaNGA: Probing the Kinematic Morphology-Density Relation of Early-type Galaxies with MaNGAen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.3847/2041-8213/aa8ace-
dc.date.eissued2017-12-13en_US
dc.identifier.eissn2041-8213-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

Files in This Item:
File Description SizeFormat 
Greene_2017_ApJL_851_L33.pdf1.18 MBAdobe PDFView/Download
Show Simple Item Record


Items in OAR@Princeton are protected by copyright, with all rights reserved, unless otherwise indicated.

Search
Browse