# A catalogue of oxygen-rich pulsating giants in the galactic halo and the   Sagittarius stream

**Authors:** Nicolas Mauron, Luc P.A. Maurin, Tim R. Kendall

arXiv: 1903.12163 · 2019-06-26

## TL;DR

This paper compiles a detailed catalogue of oxygen-rich pulsating AGB stars in the galactic halo and Sagittarius stream, using observational data to analyze their properties, distances, and distribution, revealing insights into galactic structure.

## Contribution

It presents a new, comprehensive catalogue of 417 oxygen-rich pulsating AGB stars in the galactic halo and Sagittarius stream, including their distances, velocities, and spatial distribution.

## Key findings

- Most M stars are in the Sagittarius tidal arms.
- Some stars are as distant as 150 kpc, possibly in the galactic halo.
- The catalogue includes 260 halo stars with $|Z| > 5$ kpc.

## Abstract

In order to construct a catalogue of oxygen-rich (noted M) asymptotic giant branch (AGB) stars in the halo, complementing those of carbon-rich (C) stars, previous lists of Miras and SRa semiregulars located in the nor thern hemisphere are merged and cleaned of various defects. After putting aside known C stars, characteristics lik e colours and periods indicate that most of the remaining objects are M stars. Distances are obtained through the pe riod-luminosity relation. By considering their position in the sky, stars lying at $|Z| > 5$~kpc are confirmed to b e in majority in the Sgr tidal arms. The M stars are more numerous than C ones. Our distance scale is supported by t wo cool variables located in the Pal~4 globular cluster. Along the Sgr arms, there is reasonable agreement on distan ces of our objects with recent RR Lyrae distances. A few stars may be as distant as 150~kpc, with possibly four at t he trailing arm apocenter, and two in the A16 substructure, angularly close to two C stars. Ninety radial velocities are collected from $Gaia$ and other sources. A catalogue with 417 M pulsating AGB stars is provided. It contains $\sim$ 260 stars in the halo with $|Z| > 5$~kpc. Their $K_{\rm s}$ magnitudes range from 8 u p to 13. For comparison, the catalogue also provides $\sim 150$ stars in the disc having $5$~$< K_{\rm s} <$~$8$. The catalog is available on request (NM) before being on CDS.

## Full text

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## Figures

25 figures with captions in the complete paper: https://tomesphere.com/paper/1903.12163/full.md

## References

48 references — full list in the complete paper: https://tomesphere.com/paper/1903.12163/full.md

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Source: https://tomesphere.com/paper/1903.12163