The nearby evolved stars survey II : constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
- Author
- 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, Ilse De Looze (UGent) , 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 and A A Zijlstra
- Organization
- Project
- Abstract
- The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of similar to 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 x 10(-5) M-circle dot 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 $\mu$m 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
- Space and Planetary Science, Astronomy and Astrophysics, catalogues, surveys, stars: AGB and post-AGB, stars: mass-loss, stars: winds, outflows, MASS-LOSS RATES, PERIOD-LUMINOSITY RELATION, CIRCUMSTELLAR CO EMISSION, CARBON-MONOXIDE EMISSION, REVISED AFGL CATALOGS, LOW-TEMPERATURE MIR, GIANT BRANCH STARS, AGB STARS, TP-AGB, ABSORPTION-COEFFICIENT
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Citation
Please use this url to cite or link to this publication: http://hdl.handle.net/1854/LU-8765166
- MLA
- Scicluna, P., et al. “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, 2022, pp. 1091–110, doi:10.1093/mnras/stab2860.
- APA
- Scicluna, P., Kemper, F., McDonald, I., Srinivasan, S., Trejo, A., Wallström, S. H. J., … 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
- Chicago author-date
- Scicluna, P, F Kemper, I McDonald, S Srinivasan, A Trejo, S H J Wallström, J G A Wouterloot, et al. 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.
- Chicago author-date (all authors)
- Scicluna, P, 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, Ilse 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, and A A Zijlstra. 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. doi:10.1093/mnras/stab2860.
- Vancouver
- 1.Scicluna P, Kemper F, McDonald I, Srinivasan S, Trejo A, Wallström SHJ, et al. 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. 2022;512(1):1091–110.
- IEEE
- [1]P. Scicluna et al., “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, 2022.
@article{8765166, abstract = {{The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of similar to 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 x 10(-5) M-circle dot 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 $\mu$m spectral indices are consistent with the blackbody Rayleigh-Jeans regime, suggesting a large fraction of evolved stars have unexpectedly large envelopes of cold dust.}}, author = {{Scicluna, P and Kemper, F and McDonald, I and Srinivasan, S and Trejo, A and Wallström, S H J and Wouterloot, J G A and Cami, J and Greaves, J and He, Jinhua and Hoai, D T and Kim, Hyosun and Jones, O C and Shinnaga, H and Clark, C J R and Dharmawardena, T and Holland, W and Imai, H and van Loon, J Th and Menten, K M and Wesson, R and Chawner, H and Feng, S and Goldman, S and Liu, F C and MacIsaac, H and Tang, J and Zeegers, S and Amada, K and Antoniou, V and Bemis, A and Boyer, M L and Chapman, S and Chen, X and Cho, S-H and Cui, L and Dell’Agli, F and Friberg, P and Fukaya, S and Gomez, H and Gong, Y and Hadjara, M and Haswell, C and Hirano, N and Hony, S and Izumiura, H and Jeste, M and Jiang, X and Kaminski, T and Keaveney, N and Kim, J and Kraemer, K E and Kuan, Y-J and Lagadec, E and Lee, C F and Li, D and Liu, S-Y and Liu, T and De Looze, Ilse and Lykou, F and Maraston, C and Marshall, J P and Matsuura, M and Min, C and Otsuka, M and Oyadomari, M and Parsons, H and Patel, N A and Peeters, E and Pham, T A and Qiu, J and Randall, S and Rau, G and Redman, M P and Richards, A M S and Serjeant, S and Shi, C and Sloan, G C and Smith, M W L and Suh, K-W and Toalá, J A and Uttenthaler, S and Ventura, P and Wang, B and Yamamura, I and Yang, T and Yun, Y and Zhang, F and Zhang, Y and Zhao, G and Zhu, M and Zijlstra, A A}}, issn = {{0035-8711}}, journal = {{MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY}}, keywords = {{Space and Planetary Science,Astronomy and Astrophysics,catalogues,surveys,stars: AGB and post-AGB,stars: mass-loss,stars: winds,outflows,MASS-LOSS RATES,PERIOD-LUMINOSITY RELATION,CIRCUMSTELLAR CO EMISSION,CARBON-MONOXIDE EMISSION,REVISED AFGL CATALOGS,LOW-TEMPERATURE MIR,GIANT BRANCH STARS,AGB STARS,TP-AGB,ABSORPTION-COEFFICIENT}}, language = {{eng}}, number = {{1}}, pages = {{1091--1110}}, title = {{The nearby evolved stars survey II : constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope}}, url = {{http://doi.org/10.1093/mnras/stab2860}}, volume = {{512}}, year = {{2022}}, }
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