Pith. sign in

REVIEW

The Dragonfly Edge-on Galaxies Survey: Shaping the outer disc of NGC 4565 via accretion

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1910.05358 v2 pith:FOED7A7Z submitted 2019-10-11 astro-ph.GA

The Dragonfly Edge-on Galaxies Survey: Shaping the outer disc of NGC 4565 via accretion

classification astro-ph.GA
keywords discedge-onarcsecdragonflygalaxiesgalaxyimagingnorthwest
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
Share X Bluesky LinkedIn Reddit HN
read the original abstract

We present extremely deep imaging of the well-known edge-on galaxy NGC 4565 (the "Needle Galaxy"), observed as part of the Dragonfly Edge-on Galaxies Survey. Our imaging traces starlight over scales of ~100 kpc to surface brightnesses of ~32 mag/arcsec^2 in azimuthally averaged radial profiles. In narrow slice profiles along the major axis (with bin sizes ranging from 1.7 x 0.5 kpc to 1.7 x 7.8 kpc), we achieve a depth of ~29-30 mag/arcsec^2. We confirm the previously observed asymmetric disc truncation. In addition, the sharp northwest truncation turns over to a shallower component that coincides with a fan-like feature seen to wrap around the northwest disc limb. We propose that the fan may be a tidal ribbon, and qualitatively replicate the fan with simple simulations. Alternative explanations of the fan and the disc's asymmetry are considered as well. We conclude that we are most likely seeing evidence for accretion-based outer disk growth in NGC 4565.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.