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A&A 612, L8 (2018)

Letter to the Editor

Disk stars in the Milky Way detected beyond 25 kpc from its center

M. López-Corredoira1,2, C. Allende Prieto1,2, F. Garzón1,2, H. Wang3,4, C. Liu3,4 and L. Deng3,4

1 Instituto de Astrofísica de Canarias, 38205 La Laguna, Tenerife, Spain 

2 Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain 

3 Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China 

4 University of Chinese Academy of Sciences, Beijing 100012, PR China 

Received: 22 February 2018 Accepted: 5 April 2018

Source/Fonte: NASA


Context. The maximum size of the Galactic stellar disk is not yet known. Some studies have suggested an abrupt drop-off of the stellar density of the disk at Galactocentric distances R ≳ 15 kpc, which means that in practice no disk stars or only very few of them should be found beyond this limit. However, stars in the Milky Way plane are detected at larger distances. In addition to the halo component, star counts have placed the end of the disk beyond 20 kpc, although this has not been spectroscopically confirmed so far. Aims. Here, we aim to spectroscopically confirm the presence of the disk stars up to much larger distances.

Methods. With data from the LAMOST and SDSS-APOGEE spectroscopic surveys, we statistically derived the maximum distance at which the metallicity distribution of stars in the Galactic plane is distinct from that of the halo populations.

Results. Our analysis reveals the presence of disk stars at R > 26 kpc (99.7% C.L.) and even at R > 31 kpc (95.4% C.L.).

Key words: Galaxy: structure – Galaxy: disk – Galaxy: abundances

© ESO 2018

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