English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

The isolation, simple apparent structure and low luminosity of the nearby spiral galaxy NGC 6503 make it an ideal candidate for an in‐depth kinematic and photometric study. We introduce a new publicly available code, D isk F it , that implements procedures for fitting non‐axisymmetries in either kinematic or photometric data. We use D isk F it  to analyse new Hα and CO velocity field data as well as H  i  kinematics from Greisen et al. to search for non‐circular motions in the disc of NGC 6503. We find NGC 6503 to have remarkably regular gas kinematics that are well described by rotation only. We also use D isk F it  and a new  K  s ‐band image of NGC 6503 to constrain photometric models of the disc, bar and bulge. We find the galaxy to be photometrically dominated by the disc. We find NGC 6503 to contain a faint bar and an exponential bulge which together contribute only ∼5 per cent of the total galaxy light. The combination of our kinematic and photometric D isk F it  models suggests that NGC 6503 contains a weak, end‐on bar that may have produced its Type II surface brightness profile but is unlikely to be responsible for its strong σ‐drop.

Searching for non‐axisymmetries in NGC 6503: a weak end‐on bar