中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Molecular isotopologue measurements toward super star clusters and the relation to their ages in NGC 253 with ALCHEMI

文献类型:期刊论文

作者Butterworth, J.6; Viti, S.6; Van der Werf, P. P.6; Mangum, J. G.14; Martin, S.15,16; Harada, N.17,19,21; Emig, K. L.14; Muller, S.20; Sakamoto, K.17,19; Yoshimura, Y.18
刊名ASTRONOMY & ASTROPHYSICS
出版日期2024-05-28
卷号686页码:A31
关键词astrochemistry ISM: molecules galaxies: active galaxies: ISM galaxies: starburst
ISSN号0004-6361
DOI10.1051/0004-6361/202348787
产权排序16
英文摘要Context. Determining the evolution of the CNO isotopes in the interstellar medium (ISM) of starburst galaxies can yield important constraints on the ages of super star clusters (SSCs), or on other aspects and factors contributing to their evolution, such as the initial mass function (IMF). Due to the time-dependent nature of the abundances of isotopes within the ISM - as they are supplied from processes such as nucleosynthesis or chemical fractionation -, this provides the opportunity to test whether or not isotope ratios trace the ages of highly star-forming regions, such as SSCs. Aims. The goal of this study is to investigate whether the isotopic variations in SSC regions within NGC 253 are correlated with their different ages as derived from stellar population modelling. Methods. We measured abundance ratios of CO, HCN, and HCO+ isotopologues in six regions containing SSCs within NGC 253 using high-spatial-resolution (1.6 '', similar to 28 pc) data from the ALCHEMI (ALma Comprehensive High-resolution Extragalactic Molecular Inventory) ALMA Large program. We then analysed these ratios using RADEX radiative transfer modelling, with the parameter space sampled using the nested sampling Monte Carlo algorithm MLFriends. These abundance ratios were then compared to ages predicted in each region via the fitting of observed star-formation tracers (such as Br gamma) to Starburst99 starburst stellar population evolution models. Results. We determined the isotopic column density ratios across multiple regions of SSC activity in NGC 253 using non-LTE radiative transfer modelling. We do not find any significant trend with age for the CO and HCN isotopologue ratios on timescales of the ages of the SSC* regions observed. However, HCO+ may show a correlation with age over these timescales in C-12/C-13. Conclusions. The driving factors of these ratios within SSCs could be the IMF or fractionation effects. To further probe these effects in SSCs over time, a larger sample of SSCs must be observed spanning a larger age range.
WOS关键词SUB-DOPPLER MEASUREMENTS ; MILLIMETER-WAVE OBSERVATIONS ; LUMINOUS INFRARED GALAXIES ; GALACTIC C-12/C-13 RATIOS ; ROTATIONAL SPECTRUM ; DENSE-GAS ; INTERSTELLAR-MEDIUM ; NITROGEN FRACTIONATION ; INITIAL CONDITIONS ; CENTRAL STARBURST
资助项目European Research Council (ERC) ; MCIN/AEI[PID2019-105552RB-C41] ; Consejo Superior de Investigaciones Cientificas (CSIC) ; Centro de Astrobiologia (CAB)[833460] ; [RYC2020-029387-I] ; [20225AT015]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001233655700010
出版者EDP SCIENCES S A
资助机构European Research Council (ERC) ; MCIN/AEI ; Consejo Superior de Investigaciones Cientificas (CSIC) ; Centro de Astrobiologia (CAB)
源URL[http://ir.xao.ac.cn/handle/45760611-7/6766]  
专题研究单元未命名
通讯作者Butterworth, J.
作者单位1.Keio Univ, Fac Sci & Technol, Dept Phys, 3-14-1 Hiyoshi, Yokohama, Kanagawa 2238522, Japan
2.CSIC, Inst Space Sci ICE, Campus UAB,Carrer Magrans, Barcelona 08193, Spain
3.Ctr Astrobiol CAB, CSIC INTA, Ctra Torrejon Ajalvir Km 4, Torrejon De Ardoz 28850, Madrid, Spain
4.Univ Virginia, Dept Astron, POB 400325,530 McCormick Rd, Charlottesville, VA 22904 USA
5.Max Planck Inst Radioastron, Auf-dem-Hugel 69, D-53121 Bonn, Germany
6.Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands
7.Univ British Columbia, Dept Phys & Astron, 6225 Agr Rd, Vancouver, BC V6T 1Z1, Canada
8.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
9.Tech Univ Denmark, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark
10.Cosm Dawn Ctr DAWN, Copenhagen, Denmark
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Butterworth, J.,Viti, S.,Van der Werf, P. P.,et al. Molecular isotopologue measurements toward super star clusters and the relation to their ages in NGC 253 with ALCHEMI[J]. ASTRONOMY & ASTROPHYSICS,2024,686:A31.
APA Butterworth, J..,Viti, S..,Van der Werf, P. P..,Mangum, J. G..,Martin, S..,...&Zhou, D..(2024).Molecular isotopologue measurements toward super star clusters and the relation to their ages in NGC 253 with ALCHEMI.ASTRONOMY & ASTROPHYSICS,686,A31.
MLA Butterworth, J.,et al."Molecular isotopologue measurements toward super star clusters and the relation to their ages in NGC 253 with ALCHEMI".ASTRONOMY & ASTROPHYSICS 686(2024):A31.

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