The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars

I. McDonald; S. Srinivasan; P. Scicluna; O C Jones; A. A. Zijlstra; S. H. J. Wallström; T. Danilovich; J. H. He; J. P. Marshall; J. Th van Loon; R. Wesson; F. Kemper; A. Trejo-Cruz; J. Greaves; T. Dharmawardena; J. Cami; Hyosung Kim; K. E. Kraemer; C J R Clark; H. Shinnaga; C. Haswell; H. Imai; J. G. A. Wouterloot; A. J. Pérez Vidal; G. Rau; the NESS collaboration

doi:10.1093/mnras/staf978

The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars

I. McDonald, S. Srinivasan, P. Scicluna, O C Jones , A. A. Zijlstra, S. H. J. Wallström, T. Danilovich, J. H. He, J. P. Marshall, J. Th van Loon, R. Wesson, F. Kemper, A. Trejo-Cruz, J. Greaves, T. Dharmawardena, J. Cami, Hyosung Kim, K. E. Kraemer, C J R Clark, H. ShinnagaC. Haswell, H. Imai, J. G. A. Wouterloot, A. J. Pérez Vidal, G. Rau, the NESS collaboration

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Abstract

We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the Solar Neighbourhood: (1) 852 stars from the Nearby Evolved Stars Survey (NESS), and (2) a partially overlapping set of 507 evolved stars within 300 pc. We also investigate distance determinations to these stars, their luminosity functions and their spatial distribution. Gaia APSIS GSP-Phot AENEAS temperatures of bright giant stars often appear to be underestimated. Existing literature on AGB stars under-samples both the most and least extreme nearby dust-producing stars. We reproduce the literature star-formation history of the solar neighbourhood, though stellar-evolution models over-predict the number of AGB stars of ages around 500 Myr. The distribution of AGB stars broadly matches the known 300 pc scale height of the Galactic disc and shows concentration in the direction of the Galactic centre. Most dust-producing carbon stars belong to the Galactic thick-disc population.

Original language	English
Article number	staf978
Journal	Monthly Notices of the Royal Astronomical Society (MNRAS)
DOIs	https://doi.org/10.1093/mnras/staf978
Publication status	E-pub ahead of print - 13 Jun 2025

Keywords

astro-ph.SR
astro-ph.GA

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10.1093/mnras/staf978Licence: CC BY

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© 2025 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Society. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1093/mnras/staf978
Accepted author manuscript, 2.49 MBLicence: CC BY

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McDonald, I., Srinivasan, S., Scicluna, P., Jones , O. C., Zijlstra, A. A., Wallström, S. H. J., Danilovich, T., He, J. H., Marshall, J. P., van Loon, J. T., Wesson, R., Kemper, F., Trejo-Cruz, A., Greaves, J., Dharmawardena, T., Cami, J., Kim, H., Kraemer, K. E., Clark, C. J. R., ... collaboration, T. NESS. (2025). The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars. Monthly Notices of the Royal Astronomical Society (MNRAS), Article staf978. Advance online publication. https://doi.org/10.1093/mnras/staf978

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title = "The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars",

abstract = "We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the Solar Neighbourhood: (1) 852 stars from the Nearby Evolved Stars Survey (NESS), and (2) a partially overlapping set of 507 evolved stars within 300 pc. We also investigate distance determinations to these stars, their luminosity functions and their spatial distribution. Gaia APSIS GSP-Phot AENEAS temperatures of bright giant stars often appear to be underestimated. Existing literature on AGB stars under-samples both the most and least extreme nearby dust-producing stars. We reproduce the literature star-formation history of the solar neighbourhood, though stellar-evolution models over-predict the number of AGB stars of ages around 500 Myr. The distribution of AGB stars broadly matches the known 300 pc scale height of the Galactic disc and shows concentration in the direction of the Galactic centre. Most dust-producing carbon stars belong to the Galactic thick-disc population.",

keywords = "astro-ph.SR, astro-ph.GA",

author = "I. McDonald and S. Srinivasan and P. Scicluna and Jones, \{O C\} and Zijlstra, \{A. A.\} and Wallstr{\"o}m, \{S. H. J.\} and T. Danilovich and He, \{J. H.\} and Marshall, \{J. P.\} and \{van Loon\}, \{J. Th\} and R. Wesson and F. Kemper and A. Trejo-Cruz and J. Greaves and T. Dharmawardena and J. Cami and Hyosung Kim and Kraemer, \{K. E.\} and Clark, \{C J R\} and H. Shinnaga and C. Haswell and H. Imai and Wouterloot, \{J. G. A.\} and Vidal, \{A. J. P{\'e}rez\} and G. Rau and collaboration, \{the NESS\}",

note = "{\textcopyright} 2025 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Society.",

year = "2025",

month = jun,

day = "13",

doi = "10.1093/mnras/staf978",

language = "English",

journal = "Monthly Notices of the Royal Astronomical Society (MNRAS)",

issn = "0035-8711",

publisher = "Oxford University Press (OUP)",

}

McDonald, I, Srinivasan, S, Scicluna, P, Jones , OC, Zijlstra, AA, Wallström, SHJ, Danilovich, T, He, JH, Marshall, JP, van Loon, JT, Wesson, R, Kemper, F, Trejo-Cruz, A, Greaves, J, Dharmawardena, T, Cami, J, Kim, H, Kraemer, KE, Clark, CJR, Shinnaga, H, Haswell, C, Imai, H, Wouterloot, JGA, Vidal, AJP, Rau, G & collaboration, TNESS 2025, 'The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars', Monthly Notices of the Royal Astronomical Society (MNRAS). https://doi.org/10.1093/mnras/staf978

TY - JOUR

T1 - The Nearby Evolved Stars Survey (NESS) V

T2 - properties of volume-limited samples of Galactic evolved stars

AU - McDonald, I.

AU - Srinivasan, S.

AU - Scicluna, P.

AU - Jones , O C

AU - Zijlstra, A. A.

AU - Wallström, S. H. J.

AU - Danilovich, T.

AU - He, J. H.

AU - Marshall, J. P.

AU - van Loon, J. Th

AU - Wesson, R.

AU - Kemper, F.

AU - Trejo-Cruz, A.

AU - Greaves, J.

AU - Dharmawardena, T.

AU - Cami, J.

AU - Kim, Hyosung

AU - Kraemer, K. E.

AU - Clark, C J R

AU - Shinnaga, H.

AU - Haswell, C.

AU - Imai, H.

AU - Wouterloot, J. G. A.

AU - Vidal, A. J. Pérez

AU - Rau, G.

AU - collaboration, the NESS

PY - 2025/6/13

Y1 - 2025/6/13

N2 - We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the Solar Neighbourhood: (1) 852 stars from the Nearby Evolved Stars Survey (NESS), and (2) a partially overlapping set of 507 evolved stars within 300 pc. We also investigate distance determinations to these stars, their luminosity functions and their spatial distribution. Gaia APSIS GSP-Phot AENEAS temperatures of bright giant stars often appear to be underestimated. Existing literature on AGB stars under-samples both the most and least extreme nearby dust-producing stars. We reproduce the literature star-formation history of the solar neighbourhood, though stellar-evolution models over-predict the number of AGB stars of ages around 500 Myr. The distribution of AGB stars broadly matches the known 300 pc scale height of the Galactic disc and shows concentration in the direction of the Galactic centre. Most dust-producing carbon stars belong to the Galactic thick-disc population.

AB - We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the Solar Neighbourhood: (1) 852 stars from the Nearby Evolved Stars Survey (NESS), and (2) a partially overlapping set of 507 evolved stars within 300 pc. We also investigate distance determinations to these stars, their luminosity functions and their spatial distribution. Gaia APSIS GSP-Phot AENEAS temperatures of bright giant stars often appear to be underestimated. Existing literature on AGB stars under-samples both the most and least extreme nearby dust-producing stars. We reproduce the literature star-formation history of the solar neighbourhood, though stellar-evolution models over-predict the number of AGB stars of ages around 500 Myr. The distribution of AGB stars broadly matches the known 300 pc scale height of the Galactic disc and shows concentration in the direction of the Galactic centre. Most dust-producing carbon stars belong to the Galactic thick-disc population.

KW - astro-ph.SR

KW - astro-ph.GA

U2 - 10.1093/mnras/staf978

DO - 10.1093/mnras/staf978

M3 - Article

SN - 0035-8711

JO - Monthly Notices of the Royal Astronomical Society (MNRAS)

JF - Monthly Notices of the Royal Astronomical Society (MNRAS)

M1 - staf978

ER -

The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars

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