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Chinese Academy of Sciences Institutional Repositories Grid
Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes

文献类型:期刊论文

作者Martinez-Delgado, David19,20,21; Stein, Michael18; Sakowska, Joanna D.13,14,19; Maurice Weigelt, M.; Roman, Javier12,13,14; Donatiello, Giuseppe11; Roca-Fabrega, Santi10; Schirmer, Mischa9; Grebel, Eva K.8; Saifollahi, Teymoor7
刊名ASTRONOMY & ASTROPHYSICS
出版日期2025-09-12
卷号701页码:A182
关键词methods: observational galaxies: dwarf galaxies: formation galaxies: halos galaxies: interactions
ISSN号0004-6361
DOI10.1051/0004-6361/202554980
产权排序14
英文摘要Context. Tidal interactions between massive galaxies and their satellites are fundamental processes in a universe with a Lambda cold dark matter (Lambda CDM) cosmology, and they redistribute material into faint features that preserve records of past galactic interactions. While stellar streams in the Local Group impressively demonstrate satellite disruption, they do not constitute a statistically significant sample. Constructing a substantial catalog of stellar streams beyond the Local Group remains challenging due to the difficulties in obtaining sufficiently deep wide-field images of galaxies. Despite their potential to illuminate dark matter distribution and galaxy formation processes overall, stellar streams remain underutilized as cosmological probes. Aims. The Stellar Tidal Stream Survey (STSS) addresses this observational gap by leveraging amateur telescopes to obtain deep scientific-grade images of galactic outskirts capable of building a more statistically meaningful sample of stellar streams. Methods. Over the past decade, the STSS has acquired deep (up to surface brightness limit similar to 28.3 mag/arcsec(2) in the r-band) wide-field images of 16 nearby Milky Way analog galaxies using a coordinated network of robotic amateur telescopes, which enabled the survey to avoid the issues associated with "mosaicking" smaller images taken with a single professional telescope. Results. Our survey revealed a diverse range of previously unreported faint features related to dwarf satellite accretion, including stellar streams, shells, and umbrella-like structures. We serendipitously discovered an ultra-diffuse galaxy (NGC150-UDG1) that shows hints of tidal tails. Conclusions. The STSS demonstrates the suitability of modern amateur telescopes to detect and study faint, diffuse structures in large fields around nearby spiral galaxies. Their economic and accessibility advantages enable larger statistical samples with deep imaging, which are essential for testing galaxy formation models and constraining the frequency and properties of minor merger events in the local Universe.
WOS关键词DIGITAL SKY SURVEY ; DWARF GALAXY ; STAR-FORMATION ; H-I ; DIFFUSE GALAXIES ; OUTER STRUCTURE ; GASEOUS DISKS ; DARK ENERGY ; MILKY-WAY ; NGC 5907
资助项目European Union Next Generation EU/PRTR[CNS2022-136017] ; European Union Next Generation EU/PRTR[MICIU/AEI /10.13039/501100011033] ; Governments of Spain[CEX2021-001131-S] ; Governments of Spain[MCIN/AEI/10.13039/501100011033] ; Governments of Spain[PDI2020-114581GB-C21/ AEI / 10.13039/501100011033] ; Fondo de Inversiones de Teruel ; Aragonese Government through the Research Group E16_23R ; German Science Foundation DFG, within the Collaborative Research Center[SFB1491] ; Spanish Ministry of Science and Innovation ; Max-Planck Society[PID2022-138896NB-C55] ; Max Planck Institute for Extraterrestrial Physics ; Queen's University Belfast ; National Central University of Taiwan ; Space Telescope Science Institute ; National Aeronautics and Space Administration[NNX08AR22G] ; NASA Science Mission Directorate ; National Science Foundation[AST-1238877] ; University of Maryland, Eotvos Lorand University (ELTE) ; Los Alamos National Laboratory ; Gordon and Betty Moore Foundation - Japanese Ministry of Education, Culture, Sports, Science, and Technology (MEXT) scholarship[21244012] ; Gordon and Betty Moore Foundation - Japanese Ministry of Education, Culture, Sports, Science, and Technology (MEXT) scholarship[24253003] ; European Research Council (ERC) ; Spanish Ministry of Economy and Competitiveness (MINECO)[339659-MUSICOS] ; ARC LIEF grant[AYA2016-76219-P] ; ARC LIEF grant[PID2021-124918NA-C43] ; ARC LIEF grant[ICTS-MRR-2021-03-CEFCA] ; Australian Research Council[LE130100104] ; Australian National University ; Australian Astronomical Observatory ; SkyMapper Team at ANU ; Astronomy Australia Limited (AAL) ; Australian Government through the Commonwealth's Education Investment Fund (EIF) ; National Collaborative Research Infrastructure Strategy (NCRIS) ; National eResearch Collaboration Tools and Resources (NeCTAR) ; Australian National Data Service Projects (ANDS)
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001571405400022
出版者EDP SCIENCES S A
资助机构European Union Next Generation EU/PRTR ; Governments of Spain ; Fondo de Inversiones de Teruel ; Aragonese Government through the Research Group E16_23R ; German Science Foundation DFG, within the Collaborative Research Center ; Spanish Ministry of Science and Innovation ; Max-Planck Society ; Max Planck Institute for Extraterrestrial Physics ; Queen's University Belfast ; National Central University of Taiwan ; Space Telescope Science Institute ; National Aeronautics and Space Administration ; NASA Science Mission Directorate ; National Science Foundation ; University of Maryland, Eotvos Lorand University (ELTE) ; Los Alamos National Laboratory ; Gordon and Betty Moore Foundation - Japanese Ministry of Education, Culture, Sports, Science, and Technology (MEXT) scholarship ; European Research Council (ERC) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; ARC LIEF grant ; Australian Research Council ; Australian National University ; Australian Astronomical Observatory ; SkyMapper Team at ANU ; Astronomy Australia Limited (AAL) ; Australian Government through the Commonwealth's Education Investment Fund (EIF) ; National Collaborative Research Infrastructure Strategy (NCRIS) ; National eResearch Collaboration Tools and Resources (NeCTAR) ; Australian National Data Service Projects (ANDS)
源URL[http://ir.xao.ac.cn/handle/45760611-7/8157]  
专题恒星形成与演化研究团组
通讯作者Martinez-Delgado, David
作者单位1.Doc Greiner Res Observ Rancho Hidalgo, Animas, NM USA
2.Univ Arizona, Dept Astron, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85748 USA
3.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
5.Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany
6.Tivoli Southern Sky Guest Farm, Windhoek, Namibia
7.Univ Strasbourg, CNRS, Observ Astron Strasbourg ObAS, UMR 7550, F-67000 Strasbourg, France
8.Zent Astron Univ Heidelberg, Astron Rechen Inst, Monchhofstr 12-14, D-69120 Heidelberg, Germany
9.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
10.Lund Univ, Dept Phys, Div Astrophys, Lund Observ, Box 43, SE-22100 Lund, Sweden
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Martinez-Delgado, David,Stein, Michael,Sakowska, Joanna D.,et al. Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes[J]. ASTRONOMY & ASTROPHYSICS,2025,701:A182.
APA Martinez-Delgado, David.,Stein, Michael.,Sakowska, Joanna D..,Maurice Weigelt, M..,Roman, Javier.,...&Miro-Carretero, Juan.(2025).Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes.ASTRONOMY & ASTROPHYSICS,701,A182.
MLA Martinez-Delgado, David,et al."Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes".ASTRONOMY & ASTROPHYSICS 701(2025):A182.

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