A Dwarf Disrupting -- Andromeda XXVII and the North West Stream
Janet Preston, Michelle L.M. Collins, Rodrigo A. Ibata, Erik J., Tollerud, R. Michael Rich, Ana Bonaca, Alan W. McConnachie, Dougal Mackey,, Geraint F. Lewis, Nicolas F. Martin, Jorge Pe\~narrubia, Scott C. Chapman and, Maxime Delorme

TL;DR
This study analyzes the kinematics and metallicity of stars in Andromeda XXVII and the North West Stream, suggesting a possible progenitor relationship and providing new measurements of their properties.
Contribution
It offers the first detailed spectroscopic analysis of stars in Andromeda XXVII and the North West Stream, linking the stream to its potential dwarf galaxy progenitor.
Findings
Andromeda XXVII is at 827 kpc with metallicity -2.1
North West Stream has metallicity -1.8 and shows a velocity gradient
The stream and galaxy are likely related, with the galaxy as progenitor
Abstract
We present a kinematic and spectroscopic analysis of 38 red giant branch stars, in 7 fields, spanning the dwarf spheroidal galaxy Andromeda XXVII and the upper segment of the North West Stream. Both features are located in the outer halo of the Andromeda galaxy at a projected radius of 50-80 kpc, with the stream extending for 3 on the sky. Our data is obtained as part of the PAndAS survey and enables us to confirm that Andromeda XXVII's heliocentric distance is 827 47 kpc and spectroscopic metallicity is -2.1. We also re-derive Andromeda XXVII's kinematic properties, measuring a systemic velocity = -526.1{\kms} and a velocity dispersion that we find to be non-Gaussian but for which we derive a formal value of 27.0{\kms}. In the upper segment of the North West Stream we measure mean values for the metallicity =…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
