The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

P. Scicluna; F. Kemper; I. McDonald; S. Srinivasan; A. Trejo; S. H.J. Wallström; J. G.A. Wouterloot; J. Cami; J. Greaves; Jinhua He; D. T. Hoai; Hyosun Kim; O. C. Jones; H. Shinnaga; C. J.R. Clark; T. Dharmawardena; W. Holland; H. Imai; J. Th Van Loon; K. M. Menten; R. Wesson; H. Chawner; S. Feng; S. Goldman; F. C. Liu; H. MacIsaac; J. Tang; S. Zeegers; K. Amada; V. Antoniou; A. Bemis; M. L. Boyer; S. Chapman; X. Chen; S. H. Cho; L. Cui; F. Dell'Agli; P. Friberg; S. Fukaya; H. Gomez; Y. Gong; M. Hadjara; C. Haswell; N. Hirano; S. Hony; H. Izumiura; M. Jeste; X. Jiang; T. Kaminski; N. Keaveney; J. Kim; K. E. Kraemer; Y. J. Kuan; E. Lagadec; C. F. Lee; D. Li; S. Y. Liu; T. Liu; I. De Looze; F. Lykou; C. Maraston; J. P. Marshall; M. Matsuura; C. Min; M. Otsuka; M. Oyadomari; H. Parsons; N. A. Patel; E. Peeters; T. A. Pham; J. Qiu; S. Randall; G. Rau; M. P. Redman; A. M.S. Richards; S. Serjeant; C. Shi; G. C. Sloan; M. W.L. Smith; K. W. Suh; J. A. Toalá; S. Uttenthaler; P. Ventura; B. Wang; I. Yamamura; T. Yang; Y. Yun; F. Zhang; Y. Zhang; G. Zhao; M. Zhu; A. A. Zijlstra

doi:10.1093/mnras/stab2860

The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

P. Scicluna^*, F. Kemper, I. McDonald, S. Srinivasan, A. Trejo, S. H.J. Wallström, J. G.A. Wouterloot, J. Cami, J. Greaves, Jinhua He, D. T. Hoai, Hyosun Kim, O. C. Jones, H. Shinnaga, C. J.R. Clark, T. Dharmawardena, W. Holland, H. Imai, J. Th Van Loon, K. M. MentenR. Wesson, H. Chawner, S. Feng, S. Goldman, F. C. Liu, H. MacIsaac, J. Tang, S. Zeegers, K. Amada, V. Antoniou, A. Bemis, M. L. Boyer, S. Chapman, X. Chen, S. H. Cho, L. Cui, F. Dell'Agli, P. Friberg, S. Fukaya, H. Gomez, Y. Gong, M. Hadjara, C. Haswell, N. Hirano, S. Hony, H. Izumiura, M. Jeste, X. Jiang, T. Kaminski, N. Keaveney, J. Kim, K. E. Kraemer, Y. J. Kuan, E. Lagadec, C. F. Lee, D. Li, S. Y. Liu, T. Liu, I. De Looze, F. Lykou, C. Maraston, J. P. Marshall, M. Matsuura, C. Min, M. Otsuka, M. Oyadomari, H. Parsons, N. A. Patel, E. Peeters, T. A. Pham, J. Qiu, S. Randall, G. Rau, M. P. Redman, A. M.S. Richards, S. Serjeant, C. Shi, G. C. Sloan, M. W.L. Smith, K. W. Suh, J. A. Toalá, S. Uttenthaler, P. Ventura, B. Wang, I. Yamamura, T. Yang, Y. Yun, F. Zhang, Y. Zhang, G. Zhao, M. Zhu, A. A. Zijlstra

^*Corresponding author for this work

Department of Earth Sciences (Include Institute of Marine Environmental Science and Technology)

Research output: Contribution to journal › Article › peer-review

12 Citations (Scopus)

Abstract

The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of ∼850 Galactic evolved stars within 3 kpc at (sub-)mm wavelengths, observed in the CO J = (2-1) and (3-2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to Gaia EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of 4.7 × 10-5 M⊙ yr-1 from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 μm spectral indices are consistent with the blackbody Rayleigh-Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.

Original language	English
Pages (from-to)	1091-1110
Number of pages	20
Journal	Monthly Notices of the Royal Astronomical Society
Volume	512
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stab2860
Publication status	Published - 2022 May 1

Keywords

catalogues
stars: AGB and post-AGB
stars: mass-loss
stars: winds, outflows
surveys

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.1093/mnras/stab2860

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Scicluna, P., Kemper, F., McDonald, I., Srinivasan, S., Trejo, A., Wallström, S. H. J., Wouterloot, J. G. A., Cami, J., Greaves, J., He, J., Hoai, D. T., Kim, H., Jones, O. C., Shinnaga, H., Clark, C. J. R., Dharmawardena, T., Holland, W., Imai, H., Van Loon, J. T., ... Zijlstra, A. A. (2022). The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope. Monthly Notices of the Royal Astronomical Society, 512(1), 1091-1110. https://doi.org/10.1093/mnras/stab2860

Scicluna, P, Kemper, F, McDonald, I, Srinivasan, S, Trejo, A, Wallström, SHJ, Wouterloot, JGA, Cami, J, Greaves, J, He, J, Hoai, DT, Kim, H, Jones, OC, Shinnaga, H, Clark, CJR, Dharmawardena, T, Holland, W, Imai, H, Van Loon, JT, Menten, KM, Wesson, R, Chawner, H, Feng, S, Goldman, S, Liu, FC, MacIsaac, H, Tang, J, Zeegers, S, Amada, K, Antoniou, V, Bemis, A, Boyer, ML, Chapman, S, Chen, X, Cho, SH, Cui, L, Dell'Agli, F, Friberg, P, Fukaya, S, Gomez, H, Gong, Y, Hadjara, M, Haswell, C, Hirano, N, Hony, S, Izumiura, H, Jeste, M, Jiang, X, Kaminski, T, Keaveney, N, Kim, J, Kraemer, KE, Kuan, YJ, Lagadec, E, Lee, CF, Li, D, Liu, SY, Liu, T, De Looze, I, Lykou, F, Maraston, C, Marshall, JP, Matsuura, M, Min, C, Otsuka, M, Oyadomari, M, Parsons, H, Patel, NA, Peeters, E, Pham, TA, Qiu, J, Randall, S, Rau, G, Redman, MP, Richards, AMS, Serjeant, S, Shi, C, Sloan, GC, Smith, MWL, Suh, KW, Toalá, JA, Uttenthaler, S, Ventura, P, Wang, B, Yamamura, I, Yang, T, Yun, Y, Zhang, F, Zhang, Y, Zhao, G, Zhu, M & Zijlstra, AA 2022, 'The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope', Monthly Notices of the Royal Astronomical Society, vol. 512, no. 1, pp. 1091-1110. https://doi.org/10.1093/mnras/stab2860

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title = "The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope",

abstract = "The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of ∼850 Galactic evolved stars within 3 kpc at (sub-)mm wavelengths, observed in the CO J = (2-1) and (3-2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to Gaia EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of 4.7 × 10-5 M⊙ yr-1 from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 μm spectral indices are consistent with the blackbody Rayleigh-Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.",

keywords = "catalogues, stars: AGB and post-AGB, stars: mass-loss, stars: winds, outflows, surveys",

author = "P. Scicluna and F. Kemper and I. McDonald and S. Srinivasan and A. Trejo and Wallstr{\"o}m, {S. H.J.} and Wouterloot, {J. G.A.} and J. Cami and J. Greaves and Jinhua He and Hoai, {D. T.} and Hyosun Kim and Jones, {O. C.} and H. Shinnaga and Clark, {C. J.R.} and T. Dharmawardena and W. Holland and H. Imai and {Van Loon}, {J. Th} and Menten, {K. M.} and R. Wesson and H. Chawner and S. Feng and S. Goldman and Liu, {F. C.} and H. MacIsaac and J. Tang and S. Zeegers and K. Amada and V. Antoniou and A. Bemis and Boyer, {M. L.} and S. Chapman and X. Chen and Cho, {S. H.} and L. Cui and F. Dell'Agli and P. Friberg and S. Fukaya and H. Gomez and Y. Gong and M. Hadjara and C. Haswell and N. Hirano and S. Hony and H. Izumiura and M. Jeste and X. Jiang and T. Kaminski and N. Keaveney and J. Kim and Kraemer, {K. E.} and Kuan, {Y. J.} and E. Lagadec and Lee, {C. F.} and D. Li and Liu, {S. Y.} and T. Liu and {De Looze}, I. and F. Lykou and C. Maraston and Marshall, {J. P.} and M. Matsuura and C. Min and M. Otsuka and M. Oyadomari and H. Parsons and Patel, {N. A.} and E. Peeters and Pham, {T. A.} and J. Qiu and S. Randall and G. Rau and Redman, {M. P.} and Richards, {A. M.S.} and S. Serjeant and C. Shi and Sloan, {G. C.} and Smith, {M. W.L.} and Suh, {K. W.} and Toal{\'a}, {J. A.} and S. Uttenthaler and P. Ventura and B. Wang and I. Yamamura and T. Yang and Y. Yun and F. Zhang and Y. Zhang and G. Zhao and M. Zhu and Zijlstra, {A. A.}",

note = "Publisher Copyright: {\textcopyright} 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.",

year = "2022",

month = may,

day = "1",

doi = "10.1093/mnras/stab2860",

language = "English",

volume = "512",

pages = "1091--1110",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

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TY - JOUR

T1 - The Nearby Evolved Stars Survey II

T2 - Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

AU - Scicluna, P.

AU - Kemper, F.

AU - McDonald, I.

AU - Srinivasan, S.

AU - Trejo, A.

AU - Wallström, S. H.J.

AU - Wouterloot, J. G.A.

AU - Cami, J.

AU - Greaves, J.

AU - He, Jinhua

AU - Hoai, D. T.

AU - Kim, Hyosun

AU - Jones, O. C.

AU - Shinnaga, H.

AU - Clark, C. J.R.

AU - Dharmawardena, T.

AU - Holland, W.

AU - Imai, H.

AU - Van Loon, J. Th

AU - Menten, K. M.

AU - Wesson, R.

AU - Chawner, H.

AU - Feng, S.

AU - Goldman, S.

AU - Liu, F. C.

AU - MacIsaac, H.

AU - Tang, J.

AU - Zeegers, S.

AU - Amada, K.

AU - Antoniou, V.

AU - Bemis, A.

AU - Boyer, M. L.

AU - Chapman, S.

AU - Chen, X.

AU - Cho, S. H.

AU - Cui, L.

AU - Dell'Agli, F.

AU - Friberg, P.

AU - Fukaya, S.

AU - Gomez, H.

AU - Gong, Y.

AU - Hadjara, M.

AU - Haswell, C.

AU - Hirano, N.

AU - Hony, S.

AU - Izumiura, H.

AU - Jeste, M.

AU - Jiang, X.

AU - Kaminski, T.

AU - Keaveney, N.

AU - Kim, J.

AU - Kraemer, K. E.

AU - Kuan, Y. J.

AU - Lagadec, E.

AU - Lee, C. F.

AU - Li, D.

AU - Liu, S. Y.

AU - Liu, T.

AU - De Looze, I.

AU - Lykou, F.

AU - Maraston, C.

AU - Marshall, J. P.

AU - Matsuura, M.

AU - Min, C.

AU - Otsuka, M.

AU - Oyadomari, M.

AU - Parsons, H.

AU - Patel, N. A.

AU - Peeters, E.

AU - Pham, T. A.

AU - Qiu, J.

AU - Randall, S.

AU - Rau, G.

AU - Redman, M. P.

AU - Richards, A. M.S.

AU - Serjeant, S.

AU - Shi, C.

AU - Sloan, G. C.

AU - Smith, M. W.L.

AU - Suh, K. W.

AU - Toalá, J. A.

AU - Uttenthaler, S.

AU - Ventura, P.

AU - Wang, B.

AU - Yamamura, I.

AU - Yang, T.

AU - Yun, Y.

AU - Zhang, F.

AU - Zhang, Y.

AU - Zhao, G.

AU - Zhu, M.

AU - Zijlstra, A. A.

PY - 2022/5/1

Y1 - 2022/5/1

N2 - The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of ∼850 Galactic evolved stars within 3 kpc at (sub-)mm wavelengths, observed in the CO J = (2-1) and (3-2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to Gaia EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of 4.7 × 10-5 M⊙ yr-1 from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 μm spectral indices are consistent with the blackbody Rayleigh-Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.

AB - The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of ∼850 Galactic evolved stars within 3 kpc at (sub-)mm wavelengths, observed in the CO J = (2-1) and (3-2) rotational lines, and the sub-mm continuum, using the James Clark Maxwell Telescope and Atacama Pathfinder Experiment. NESS consists of five tiers, based on distances and dust-production rate (DPR). We define a new metric for estimating the distances to evolved stars and compare its results to Gaia EDR3. Replicating other studies, the most-evolved, highly enshrouded objects in the Galactic Plane dominate the dust returned by our sources, and we initially estimate a total DPR of 4.7 × 10-5 M⊙ yr-1 from our sample. Our sub-mm fluxes are systematically higher and spectral indices are typically shallower than dust models typically predict. The 450/850 μm spectral indices are consistent with the blackbody Rayleigh-Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.

KW - catalogues

KW - stars: AGB and post-AGB

KW - stars: mass-loss

KW - stars: winds, outflows

KW - surveys

UR - http://www.scopus.com/inward/record.url?scp=85128855161&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85128855161&partnerID=8YFLogxK

U2 - 10.1093/mnras/stab2860

DO - 10.1093/mnras/stab2860

M3 - Article

AN - SCOPUS:85128855161

SN - 0035-8711

VL - 512

SP - 1091

EP - 1110

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

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