The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
Article
Article Title | The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope |
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ERA Journal ID | 1074 |
Article Category | Article |
Authors | Scicluna, P., Kemper, F., McDonald, I., Srinivasan, S., Trejo, A., Wallstrom, S. H. J., Wouterloot, J. G. A., Cami, J., Greaves, J., He, Jinhua, Hoai, D. T., Kim, Hyosun, Jones, O. C., Shinnaga, H., Clark, C. J. R., Dharmawardena, T., Holland, W., Imai, H., van Loon, J. Th., Menten, K. M., Wesson, R., Chawner, H., Feng, S., Goldman, S., Liu, F. C., MacIsaac, H., Tang, J., Zeegers, S., Amada, K., Antoniou, A., Bemis, A., Boyer, M. L., Chapman, S., Chen, X., Cho, S.-H., 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, K. E., Kuan, Y.-J., Lagadec, E., Lee, C. F., Li, D., Liu, S.-Y., Liu, T., de Looze, I.d., Lykou, F., Maraston, C., Marshall, J. P., Matsuura, M., Min, C., Otsuka, M., Oyadomari, M., Parsons, H., Patel, N. A., Peeters, E., Pham, T. A., Qiu, J., Randall, S., Rau, G., Redman, M. P., Richards, A. M. S., Serjeant, S., Shi, C., Sloan, G.C., Smith, M. W. L., Suh, K.-W., Toal, J. A., Uttenthaler, S., Ventura, P., wang, B., Yamamura, I., Yang, T., Yun, Y., Zhang, F., Zhang, Y., Zhao, G., Zhu, M. and Zijlstra, A. A. |
Journal Title | Monthly Notices of the Royal Astronomical Society |
Journal Citation | 512 (1), pp. 1091-1110 |
Number of Pages | 20 |
Year | 2022 |
Publisher | Oxford University Press |
ISSN | 0035-8711 |
1365-2966 | |
Digital Object Identifier (DOI) | https://doi.org/10.1093/mnras/stab2860 |
Web Address (URL) | https://academic.oup.com/mnras/article-abstract/512/1/1091/6549936?redirectedFrom=fulltext |
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 |
Keywords | stars: winds, outflows; catalogues; surveys; stars: AGB and post-AGB; stars: mass-loss |
Public Notes | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2022 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Byline Affiliations | Academia Sinica Institute of Astronomy and Astrophysics, Taiwan |
European Southern Observatory (ESO), Chile | |
European Southern Observatory (ESO), Germany | |
University of Manchester, United Kingdom | |
Open University, United Kingdom | |
Institute of Radio Astronomy and Astrophysics, Mexico | |
Institute of Astronomy, Belgium | |
East Asian Observatory, United States | |
University of Western Ontario, Canada | |
SETI Institute, United States | |
Cardiff University, United Kingdom | |
Chinese Academy of Sciences, China | |
University of Chile, Chile | |
Vietnam Academy of Science and Technology, Vietnam | |
Korea Astronomy and Space Science Institute, Korea | |
Royal Observatory Edinburgh, United Kingdom | |
Kagoshima University, Japan | |
Space Telescope Science Institute, United States | |
Max Planck Institute for Astronomy, Germany | |
Keele University, United Kingdom | |
University College London, United Kingdom | |
National Astronomical Observatory of China, China | |
National Taiwan Normal University, Taiwan | |
Texas Tech University, United States | |
Center for Astrophysics Harvard and Smithsonian, United States | |
McMaster University, Canada | |
Dalhousie University, Canada | |
INAF - Astronomical Observatory of Rome, Italy | |
Heidelberg University, Germany | |
Subaru Telescope, Japan | |
Xiamen University, China | |
National University of Ireland Galway, Ireland | |
Boston College, United States | |
University of Nice Sophia Antipolis, France | |
University of Chinese Academy of Sciences, China | |
University of Gent, Belgium | |
University of Hong Kong, China | |
University of Portsmouth, United Kingdom | |
Centre for Astrophysics | |
Graduate University for Advanced Studies, Japan | |
Kyoto University, Japan | |
Nanjing University, China | |
NASA Goddard Space Flight Center, United States | |
Catholic University of America, United States | |
Hainan University, China | |
University of North Carolina, United States | |
Chungbuk National University, Korea | |
Kuffner Observatory, Austria | |
Institute of Space and Astronautical Science, Japan | |
Sun Yat-sen University, China |
https://research.usq.edu.au/item/z02qv/the-nearby-evolved-stars-survey-ii-constructing-a-volume-limited-sample-and-first-results-from-the-james-clerk-maxwell-telescope
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