Vertaisarvioitu alkuperäisartikkeli tai data-artikkeli tieteellisessä aikakauslehdessä (A1)

Galaxy and Mass Assembly (GAMA): The Weak Environmental Dependence of Quasar Activity at 0.1 < z < 0.35

Julkaisun tekijät: Wethers CF, Acharya N, De Propris R, Kotilainen J, Baldry IK, Brough S, Driver SP, Graham AW, Holwerda BW, Hopkins AM, Lopez-Sanchez AR, Loveday J, Phillipps S, Pimbblet KA, Taylor E, Wang LY, Wright AH

Kustantaja: IOP Publishing Ltd

Julkaisuvuosi: 2022

Journal: Astrophysical Journal

Tietokannassa oleva lehden nimi: ASTROPHYSICAL JOURNAL

Lehden akronyymi: ASTROPHYS J

Volyymi: 928

Julkaisunumero: 2

Sivujen määrä: 16

ISSN: 0004-637X

eISSN: 1538-4357



Rinnakkaistallenteen osoite:

Understanding the connection between nuclear activity and galaxy environment remains critical in constraining models of galaxy evolution. By exploiting the extensive cataloged data from the Galaxy and Mass Assembly survey, we identify a representative sample of 205 quasars at 0.1 < z < 0.35 and establish a comparison sample of galaxies, closely matched to the quasar sample in terms of both stellar mass and redshift. On scales <1 Mpc, the galaxy number counts and group membership of quasars appear entirely consistent with those of the matched galaxy sample. Despite this, we find that quasars are similar to 1.5 times more likely to be classified as the group center, indicating a potential link between quasar activity and cold gas flows or galaxy interactions associated with rich group environments. On scales of similar to a few Mpc, the clustering strengths of both samples are statistically consistent, and beyond 10 Mpc, we find no evidence that quasars trace large-scale structures any more than the galaxy control sample. Both populations are found to prefer intermediate-density sheets and filaments to either very high-density environments or very low-density environments. This weak dependence of quasar activity on galaxy environment supports a paradigm in which quasars represent a phase in the lifetime of all massive galaxies and in which secular processes and a group-centric location are the dominant triggers of quasars at low redshift.

Ladattava julkaisu

This is an electronic reprint of the original article.
This reprint may differ from the original in pagination and typographic detail. Please cite the original version.

Last updated on 2022-20-05 at 13:47