GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866911232389283840 |
|---|---|
| author | Khanna, Shourya Yu, Jie Drimmel, Ronald Poggio, Eloisa Cantat-Gaudin, Tristan Castro-Ginard, Alfred Kurbatov, Evgeny Belokurov, Vasily Brown, Anthony Fouesneau, Morgan Casey, Andrew Rix, Hans-Walter |
| author_facet | Khanna, Shourya Yu, Jie Drimmel, Ronald Poggio, Eloisa Cantat-Gaudin, Tristan Castro-Ginard, Alfred Kurbatov, Evgeny Belokurov, Vasily Brown, Anthony Fouesneau, Morgan Casey, Andrew Rix, Hans-Walter |
| contents | We present an exploration of the Milky Way's structural parameters using an all-sky sample of RC giants to map the stellar density from the Galactic disc beyond 3 kpc. These evolved giants are considered to be standard candles due to their low intrinsic variance in their absolute luminosities, allowing us to estimate their distances with reasonable confidence. We exploit all-sky photometry from the AllWISE mid-infrared survey and the Gaia survey, along with astrometry from Gaia Data Release 3 and recent 3D extinction maps, to develop a probabilistic scheme in order to select with high confidence RC-like stars. Our curated catalogue contains about 10 million sources, for which we estimate photometric distances based on the WISE W1 photometry. We then derive the selection function for our sample, which is the combined selection function of sources with both Gaia and AllWISE photometry. Using the distances and accounting for the full selection function of our observables, we are able to fit a two-disc, multi-parameter model to constrain the scale height (hz), scale-length (rd), flaring, and the relative mass ratios of the two disc components. We illustrate and verify our methodology using mock catalogues of RC stars. We find that the RC population is best described by a flared disc with scale length rd=$4.24\pm0.32$ kpc and scale height at the Sun of hz(at Sun)=$0.18\pm0.01$ kpc, and a shorter and thicker disc with rd=$2.66\pm0.11$ kpc, hz(at Sun)=$0.48\pm0.11$ kpc, with no flare. The thicker disc constitutes 66\% of the RC stellar mass beyond 3 kpc, while the flared disc shows evidence of being warped beyond 9 kpc from the Galactic center. The residuals between the predicted number density of RC stars from our axisymmetric model and the measured counts show possible evidence of a two-armed spiral perturbation in the disc of the Milky Way. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_22036 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump Khanna, Shourya Yu, Jie Drimmel, Ronald Poggio, Eloisa Cantat-Gaudin, Tristan Castro-Ginard, Alfred Kurbatov, Evgeny Belokurov, Vasily Brown, Anthony Fouesneau, Morgan Casey, Andrew Rix, Hans-Walter Astrophysics of Galaxies We present an exploration of the Milky Way's structural parameters using an all-sky sample of RC giants to map the stellar density from the Galactic disc beyond 3 kpc. These evolved giants are considered to be standard candles due to their low intrinsic variance in their absolute luminosities, allowing us to estimate their distances with reasonable confidence. We exploit all-sky photometry from the AllWISE mid-infrared survey and the Gaia survey, along with astrometry from Gaia Data Release 3 and recent 3D extinction maps, to develop a probabilistic scheme in order to select with high confidence RC-like stars. Our curated catalogue contains about 10 million sources, for which we estimate photometric distances based on the WISE W1 photometry. We then derive the selection function for our sample, which is the combined selection function of sources with both Gaia and AllWISE photometry. Using the distances and accounting for the full selection function of our observables, we are able to fit a two-disc, multi-parameter model to constrain the scale height (hz), scale-length (rd), flaring, and the relative mass ratios of the two disc components. We illustrate and verify our methodology using mock catalogues of RC stars. We find that the RC population is best described by a flared disc with scale length rd=$4.24\pm0.32$ kpc and scale height at the Sun of hz(at Sun)=$0.18\pm0.01$ kpc, and a shorter and thicker disc with rd=$2.66\pm0.11$ kpc, hz(at Sun)=$0.48\pm0.11$ kpc, with no flare. The thicker disc constitutes 66\% of the RC stellar mass beyond 3 kpc, while the flared disc shows evidence of being warped beyond 9 kpc from the Galactic center. The residuals between the predicted number density of RC stars from our axisymmetric model and the measured counts show possible evidence of a two-armed spiral perturbation in the disc of the Milky Way. |
| title | GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2410.22036 |